paper_id stringlengths 9 15 | title stringlengths 0 95.9k | authors listlengths 0 639 | abstract stringlengths 0 62k | latex listlengths 0 268 | bibtex listlengths 0 7 |
|---|---|---|---|---|---|
astro-ph0001001 | Statistics of Turbulence from Spectral-Line Data Cubes | [
{
"author": "Alex Lazarian"
}
] | Emission in spectral lines can provide unique information on interstellar turbulence. Doppler shifts due to supersonic motions contain information on turbulent velocity field which is otherwise difficult to measure. However, the problem of separation of velocity and density fluctuations is far from being trivial. Using... | [
{
"name": "procl.tex",
"string": "%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n%\t\t\tprocl.tex\t\t\t%\n%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n\n\\documentstyle[procl]{article}\n\n\\input{psfig.sty}\n\n% A useful Journal macro\n\\def\\Journal#1#2#3#4{(#1) {#2} {\\bf #3}, #4... | [
{
"name": "astro-ph0001001.extracted_bib",
"string": "\\begin{thebibliography}{99}\n\\bibitem{} Adler, D. S. \\& Roberts, W. W. Jr. \\Journal{1992}{\\ApJ}{384}{95}\n\\bibitem{} Armstrong, J.M., Rickett, B.J., \\& Spangler, S.R.\n\\Journal{1995}{\\ApJ}{443}{209}\n\\bibitem{} Brand, P. \\& Wouterloot, J.G.A. ... |
astro-ph0001002 | On the inverse Compton scattering model of radio pulsars | [
{
"author": "G. J. Qiao$^{1,2}$"
},
{
"author": "R. X. Xu$^{1,2}$"
},
{
"author": "J. F. Liu$^{1,2}$"
},
{
"author": "J. L. Han$^{1,3}$"
},
{
"author": "B. Zhang$^{1,2}$"
}
] | Some characteristics of the inverse Compton scattering (ICS) model are reviewed. At least the following properties of radio pulsars can be reproduced in the model: core or central emission beam, one or two hollow emission cones, different emission heights of these components, diverse pulse profiles at various frequenci... | [
{
"name": "qHK.tex",
"string": "\\documentstyle[11pt,newpasp,twoside]{article}\n\\pagestyle{myheadings}\n\\markboth{{\\it Qiao et. al.}}{{\\it ICS model of Pulsars}}\n\\begin{document}\n\n\\title{On the inverse Compton scattering model of radio pulsars}\n\n\\author{G. J. Qiao$^{1,2}$,\n R. X. Xu$^{1,... | [
{
"name": "astro-ph0001002.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem{} Beskin, V.S., Gurevich, A.V., Istomin, Y.N., 1988,\n Ap\\&SS, 146, 205\n\n\\bibitem{} Liu, J.F., Qiao, G.J., Xu, R.X., 1999,\n Chin. Phys. Lett., 16, 541\n\n\\bibitem{} Lyne A.G., Manchester R.N., 1988,\n ... |
astro-ph0001003 | Dark Halo and Disk Galaxy Scaling Laws in Hierarchical Universes | [
{
"author": "Julio F. Navarro\\altaffilmark{1}"
}
] | % We use cosmological N-body/gasdynamical simulations that include star formation and feedback to examine the proposal that scaling laws between the total luminosity, rotation speed, and angular momentum of disk galaxies reflect analogous correlations between the structural parameters of their surrounding dark matter h... | [
{
"name": "tfemapj.tex",
"string": "\\documentstyle[emulateapj]{article}\n\\singlespace\n%\\tighten\n%\\eqsecnum\n%\n% Macros\n%\n%\\newcommand{\\etal}{{et Pl.} \\thinspace}\n\\newcommand{\\etal}{{et al.~}}\n\\newcommand{\\eg}{{e.g.,} \\thinspace}\n\\newcommand{\\ie}{{i.e.,} \\thinspace}\n\\newcommand{\\Ms... | [
{
"name": "astro-ph0001003.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[]{} Barnes, J., Efstathiou, G., 1987, \\apj, 319, 575\n%\n\\bibitem[]{} Cole, S.M., Arag\\'on-Salamanca, A., Frenk, C.S., Navarro, J.F., \\& Zepf,\nS.E.\\ 1994, \\mnras, 271, 781\n%\n\\bibitem[]{} Cole S., \\& Lace... |
astro-ph0001004 | Theory of the Interaction of Planetary Nebulae with the Interstellar Medium | [
{
"author": "Ruth Dgani"
}
] | The theory of the interaction of planetary nebulae with the interstellar medium is important for the interpretation of nebular morphologies that deviate from point symmetry. It can be used to probe the interstellar medium and its magnetic field. We emphasize in this review the role of hydrodynamical instabilities in th... | [
{
"name": "dgani.tex",
"string": "\\documentstyle[11pt,newpasp,twoside]{article}\n\\markboth{ Ruth Dgani}{Interaction of Planetary Nebulae with the Interstellar Medium}\n\\pagestyle{myheadings}\n\\nofiles\n\n% Some definitions I use in these instructions.\n\n\\def\\emphasize#1{{\\sl#1\\/}}\n\\def\\arg#1{{\\... | [] |
astro-ph0001005 | [] | [] | [] | ||
astro-ph0001006 | On the Clustering of GRBs on the Sky | [
{
"author": "Shiv K. Sethi$^1$"
},
{
"author": "S. G. Bhargavi$^2$"
},
{
"author": "and Jochen Greiner$^3$"
}
] | The two-point correlation of the 4th (current) BATSE catalog (2494 objects) is calculated. It is shown to be consistent with zero at nearly all angular scales of interest. Assuming that GRBs trace the large scale structure in the universe we calculate the angular correlation function for the standard CDM (sCDM) model. ... | [
{
"name": "GP46.tex",
"string": "\\documentstyle[epsfig]{aipproc}\n\n\\begin{document}\n\n\\title{On the Clustering of GRBs on the Sky}\n\n\\author{Shiv K. Sethi$^1$, S. G. Bhargavi$^2$, and Jochen Greiner$^3$}\n \\address{$^1$Mehta Research Institute, \nChhatnag Road, Jhusi \\\\Allahabad 221 506, India \\\... | [
{
"name": "astro-ph0001006.extracted_bib",
"string": "\\bibitem{greiner}Greiner, J. , {\\tt http://www.aip.de/People/JGreiner/grbgen.html} (1999).\n \n\\bibitem{blum} Blumenthal, G. R., Hartmann, D. H., \\& Linder, E. V. , \n {\\it AIP}, vol 307, p.117, New York (1994).\n\n\\bibitem{hart} Hartmann, D. H. ... |
astro-ph0001007 | Wide Field CCD Surface Photometry of the Giant Elliptical Galaxy NGC 4472 in the Virgo Cluster | [
{
"author": "Eunhyeuk Kim"
},
{
"author": "$^1$ Myung Gyoon Lee"
},
{
"author": "$^1$Department of Astronomy"
},
{
"author": "Seoul 151-742"
},
{
"author": "Korea"
},
{
"author": "$^2$Departamento de F\\'{\\i}sica"
},
{
"author": "Universidad de Concepci\\'on"
}... | We present deep wide field ($16'.4 \times 16'.4$ ) Washington $CT_1$ CCD surface photometry of the giant elliptical galaxy NGC 4472, the brightest member in the Virgo cluster. Our data cover a wider field than any previous CCD photometry as well as going deeper. Surface brightness profiles of NGC 4472 are not well fit ... | [
{
"name": "Kim_m49surf.tex",
"string": "% mnsample.tex\n%% Author: Eunhyeuk Kim, Myung Gyoon Lee and Doug Geisler\n%% (Seoul National University, Department of Astronomy, Seoul 151-742, Korea)\n%% Email: ekim@astro.snu.ac.kr, mglee@astrog.snu.ac.kr\n%% Title: Wide Field CCD Surface Photometry \n%% of... | [
{
"name": "astro-ph0001007.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem[Barsony 1989]{bar89} Barsony, M. 1989, PhD Thesis, Caltech \n\\bibitem[Bender \\& M\\\"ollenhoff 1987]{ben87} Bender, R., \\& M\\\"ollenhoff, C. 1987,\nA\\&A, 177, 71\n\\bibitem[Boroson \\& Thompson 1987]{bor87} Boro... |
astro-ph0001008 | [] | \noindent{In 1997 the first optical afterglow of a cosmic Gamma-Ray Burst was discovered, and substantial progress has been achieved since then. Here we present a short review of some recent developments in this field, with emphasis on observational aspects of the GRB phenomenon.} | [
{
"name": "astro-ph0001008.tex",
"string": "\\NeedsTeXFormat{LaTeX2e}\n\\documentclass[twoside]{article}\n\\usepackage[latin1]{inputenc}\n\\usepackage{t1enc}\n\\usepackage{a4}\n\\usepackage{tabularx}\n\\usepackage{epsf}\n\n\\textheight=194mm\n\\textwidth=118mm\n\\oddsidemargin=-7mm\n\\evensidemargin=-7mm\n\... | [] | |
astro-ph0001009 | THE NATURE OF ULTRA-LUMINOUS COMPACT\\ X-RAY SOURCES IN NEARBY SPIRAL GALAXIES | [
{
"author": "Kazuo {\\sc Makishima}"
},
{
"author": "Aya {\\sc Kubota}"
},
{
"author": "Tsunefumi {\\sc Mizuno}"
},
{
"author": "Tomohisa {\\sc Ohnishi}"
},
{
"author": "and Makoto {\\sc Tashiro}"
}
] | Studies were made of {ASCA} spectra of seven ultra-luminous compact X-ray sources (ULXs) in nearby spiral galaxies; M33 X-8 (Takano et al. 1994), M81 X-6 (Fabbiano 1988b; Kohmura et al. 1994; Uno 1997), IC~342 Source~1 (Okada et al. 1998), Dwingeloo~1 X-1 (Reynolds et al. 1997), NGC~1313 Source~B (Fabbiano \& Trinchier... | [
{
"name": "ms.tex",
"string": "\\documentstyle[12pt,aasms4,psfig]{article}\n%\\documentstyle[12pt,aasms4]{article}\n\\renewcommand{\\baselinestretch}{1.0}\n\\setlength{\\topmargin}{-1.0cm}\n\\setlength{\\oddsidemargin}{-0.5cm}\n\\setlength{\\evensidemargin}{-0.5cm}\n\\setlength{\\textheight}{24.5cm}\n\\setl... | [
{
"name": "astro-ph0001009.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\setlength{\\itemsep}{-1mm}\\setlength{\\baselineskip}{-6mm}\n\\bibitem[]{} Abramowicz, M.A., Czerny, B., Lasota, P., \\& Szuszkiewicz, E. 1988, \n ApJ, 332, 646\n\\bibitem[]{} Asaoka, I. 1989, PASJ, 41, 763\n\\bi... |
astro-ph0001010 | Feedback Processes in the Early Universe | [
{
"author": "A. Ferrara\\inst{1}"
},
{
"author": "B. Ciardi\\inst{2}"
},
{
"author": "S. Marri\\inst{3}"
},
{
"author": "P. Todini \\inst{2}"
}
] | Feedback effects due to massive stars and supernovae in the first objects are shown to strongly regulate both galaxy formation/evolution and the reionization process. Here we review the most important ones in some detail. We discuss how Type II supernovae can be used as tracers of the first objects and detected with NG... | [
{
"name": "esa99.tex",
"string": "%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n%\n% sample.tex -- ESLAB Conference Proceedings tutorial paper\n% ----------------------------------------------------------\n% Lines starting with \"%\" are comments; they will be ignored... | [
{
"name": "astro-ph0001010.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[\\protect \\astroncite{}{}]{}\nAbel, T., Anninos, P., Zhang, Y. \\& Norman, M. L. 1997, NewA, 2, 181\n\n\\bibitem[\\protect \\astroncite{}{}]{}\nCiardi, B., Ferrara, A. \\& Abel, T. 2000, ApJ, in press\n\n\\bibit... |
astro-ph0001011 | What can BeppoSAX tell us about short GRBs: An update from the Subsecond GRB Project | [
{
"author": "G.~Gandolfi$^{(1)}$ M.J.S.~Smith$^{(2),(4)}$ A.~Coletta$^{(2)}$ G.~Celidonio$^{(2)}$ L.~Di Ciolo$^{(2)}$ A.~Paolino$^{(2)}$ G.~Tarei$^{(2)}$ G.~Tassone$^{(2)}$ J.M.~Muller$^{(2),(4)}$ E.~Costa$^{(1)}$ M.~Feroci$^{(1)}$ F.~Frontera$^{(3),(5)}$ L.~Piro$^{(1)}$"
}
] | We present some statistical considerations on the BeppoSAX hunt for subsecond GRBs at the Scientific Operation Center. Archive analysis of a BATSE/SAX sub-sample of bursts indicates that the GRB Monitor is sensitive to short ($\le$ 2 sec) events, that are in fact $\approx$ 22$\%$ of the total. The non-detection of corr... | [
{
"name": "IP-09new.tex",
"string": "\\documentstyle{aipproc}\n\\input epsf \n\\def\\grad{$^\\circ$}\n\\begin{document}\n\\title{What can BeppoSAX tell us about short GRBs: An update from the Subsecond GRB Project}\n\n\\author{G.~Gandolfi$^{(1)}$ M.J.S.~Smith$^{(2),(4)}$ A.~Coletta$^{(2)}$ G.~Celidoni... | [
{
"name": "astro-ph0001011.extracted_bib",
"string": "\\bibitem{coletta}Coletta~A. et al. \n{\\it Proc. of the Active X-Ray Sky Workshop}, Roma, Nuclear Physics B 69/1-3, 712 (1998)\n\n\\bibitem{cline} Cline~D.B. et al. {\\it astro-ph/9905346} (1999)\n\n\\bibitem{feroci}Feroci~F. et. al. these proceedings\... |
astro-ph0001012 | Observed Properties of Mass Loss in Symbiotic Binaries | [
{
"author": "Joanna Miko{\\l}ajewska"
}
] | Both the red giants and the Mira variables in symbiotic systems have systematically higher mass-loss rates than do typical galactic giants and Miras, which suggests that only very evolved giants, and so those with highest mass-loss rates, can support symbiotic behaviour in widely separated binary systems. They often sh... | [
{
"name": "apn-talk.tex",
"string": "\\documentstyle[11pt,newpasp,twoside,epsf]{article}\n\n\\markboth{J. Miko{\\l}ajewska}{Mass Loss in Symbiotic Binary Stars}\n\\pagestyle{myheadings}\n\n%\\setcounter{page}{}\n\n\\begin{document}\n\n\\title{Observed Properties of Mass Loss in Symbiotic Binaries}\n\n\\auth... | [] |
astro-ph0001013 | Formation of Millisecond Pulsars with Heavy White Dwarf Companions.\\ Extreme Mass Transfer on Sub-Thermal Timescales | [
{
"author": "Thomas M. Tauris\\altaffilmark{1}"
},
{
"author": "Edward P. J. van den Heuvel\\altaffilmark{1}"
},
{
"author": "Gerrit J. Savonije\\altaffilmark{1}"
}
] | We have performed detailed numerical calculations of the non-conservative evolution of close {X}-ray binary systems with intermediate-mass (2.0 -- 6.0$\,M_{\odot}$) donor stars and a $1.3\,M_{\odot}$ accreting neutron star. We calculated the thermal response of the donor star to mass loss, in order to determine its sta... | [
{
"name": "letter.tex",
"string": "\\documentstyle[emulateapj,apjfonts,psfig]{article}\n\\def\\deg{\\ifmmode^{\\circ}\\;\\else$^{\\circ}\\;$\\fi} % overwrites \\deg in LaTeX\n\n\\righthead{FORMATION OF MILLISECOND PULSARS WITH HEAVY WHITE DWARF COMPANIONS}\n\\lefthead{TAURIS, VAN DEN HEUVEL \\& SAVONIJE}\n\... | [] |
astro-ph0001014 | SPIN-ORBIT COUPLINGS IN X-RAY BINARIES | [
{
"author": "T.M. TAURIS \\& G.J. SAVONIJE"
}
] | We discuss the influence of tidal spin-orbit interactions on the orbital dynamics of close intermediate-mass {X}-ray binaries. In particular we consider here a process in which spin angular momentum of a contracting RLO donor star, in a synchronous orbit, is converted into orbital angular momentum and thus helps to sta... | [
{
"name": "text.tex",
"string": "\\documentstyle[editedvolume,psfig]{crckapb} \n\n\\newcommand{\\stt}{\\small\\tt}\n\\newcommand{\\pdrv}[2]{\\frac{\\partial #1}{\\partial #2}}\n\\newcommand{\\drv}[2]{{{{\\rm d} #1}\\over {{\\rm d} #2}}}\n\\begin{opening}\n\\title{SPIN-ORBIT COUPLINGS IN X-RAY BINARIES}\n\\s... | [
{
"name": "astro-ph0001014.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem[]{} Landau L.D., Lifshitz E., 1958, The Classical Theory\n of Fields, Pergamon Press, Oxford\n\\bibitem[]{} Pratt J.P., Strittmatter P.A., 1976,\n ApJ. 204, L29\n\\bibitem[]{} Rappaport S.A., Ve... |
astro-ph0001015 | New Direct Observational Evidence for Kicks in SNe | [
{
"author": "T. M. Tauris \\& E. P. J. van den Heuvel"
}
] | [
{
"name": "paper.tex",
"string": "\\documentstyle[11pt,newpasp,twoside,epsf]{article} \n\\markboth{Tauris \\& van den Heuvel}{Evidence for Kicks}\n\\pagestyle{myheadings}\n\\begin{document}\n\\title{New Direct Observational Evidence for Kicks in SNe}\n\\author{T. M. Tauris \\& E. P. J. van den Heuvel}\n\n\\... | [
{
"name": "astro-ph0001015.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem[]{} Dewey R. J., Cordes J. M., 1987, ApJ. 321, 780\n\\bibitem[]{} Flannery B.P., van den Heuvel E.P.J., 1975, A\\&A 39, 61 \n\\bibitem[]{} Johnston H. M., Fender R. P., Wu K., 1999, MNRAS 308, 415 \n\\bibitem[]{} Kas... | |
astro-ph0001016 | The Space Density of Primordial Gas Clouds near Galaxies and Groups and their Relation to Galactic HVCs | [
{
"author": "Martin A. Zwaan and Frank H. Briggs"
}
] | The Arecibo \hi\ Strip Survey probed the halos of $\sim$300 cataloged galaxies and the environments of $\sim$14 groups with sensitivity to neutral hydrogen masses $\geq 10^{7}~\msol$. The survey detected no objects with properties resembling the High Velocity Clouds (HVCs) associated with the Milky Way or Local Group. ... | [
{
"name": "hvcs_pp.tex",
"string": "%\\documentclass{aastex} \n%\\documentclass[preprint]{aastex} \n\\documentclass[preprint2]{aastex}\n%\\documentstyle[11pt,aas2pp4,epsf,natbib]{article}\n\n\\usepackage{epsf}\n\n\\slugcomment{{\\em Accepted for publication the Astrophysical Journal Letters}} \n\n%\\shortau... | [
{
"name": "astro-ph0001016.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem[Bland-Hawthorn et al.(1998)]{bla98}Bland-Hawthorn, J.,\n Veilleux, S., Cecil, G.~N., Putman, M.~E., Gibson, B.~K., \\& \n Maloney, P.~R. 1998, \\mnras, 299, 611\n\\bibitem[Bland-Hawthorn \\& Maloney(1999)]{bla99}... |
astro-ph0001017 | H$_{2}$ emission from CRL 618 | [
{
"author": "et al."
}
] | We present a complete study of the \Htwo infrared emission, including the pure rotational lines, of the proto Planetary Nebulae CRL 618 with the ISO SWS. A large number of lines are detected. The analysis of our observations shows: (i) an OTP ratio very different from the classical value of 3, probably around 1.76-1.87... | [
{
"name": "herpin.tex",
"string": "% sample.tex -- sample pages for CUP conference proceedings style file\n%\n% Where you see \\ifx\\CUP@mtlplain@loaded\\undefined,\n% this is an internal font switch for Cambridge University Press. \n\n\\documentstyle[psfig]{cupconf}\n\n% use these four lines when finally p... | [
{
"name": "astro-ph0001017.extracted_bib",
"string": "\\begin{thebibliography}{} \n%\\bibitem[]{1984}\n%{\\sc Beckwith, S., Beck, S.C., Gatley, I.} 1984 {\\it Astrophys. Journal} \n%{\\bf 280}, 648. \n\\bibitem[]{1987}\n{\\sc Black, J.H.} 1987 {\\it Astrophys. Journal} {\\bf 322}, 412. \n\\bibitem []{1986... |
astro-ph0001018 | DO AGB STARS DIFFER CHEMICALLY FROM RGB STARS IN GLOBULAR CLUSTERS? | [
{
"author": "CHRISTOPHER SNEDEN$^1$"
},
{
"author": "INESE I. IVANS$^1$"
},
{
"author": "ROBERT P. KRAFT$^2$"
}
] | The recent improvements in globular cluster colour-magnitude diagrams, coupled with an increase in large-sample spectroscopic abundance studies of cluster giants, finally allow some attempts at a statistically meaningful comparison of the chemical compositions of red giant branch and asymptotic branch cluster stars. We... | [
{
"name": "finalagb.tex",
"string": "% TEMPLATE FILE memsait.tex TO PREAPARE CAMERA-READY PAPERS FOR\n% MEMORIE DELLA SOCIETA` ASTRONOMICA ITALIANA.\n\n% NEEDS THE FILE memsait.sty TO RUN.\n\n% MODIFIED BY A. COMASTRI IN DECEMBER 1996 TO ALLOW INCLUSION OF\n% FIGURES AND TABLES. NEEDS THE FILE epsf.sty TO R... | [
{
"name": "astro-ph0001018.extracted_bib",
"string": "\\begin{thebibliography}{} \n\n\\item Briley, M. M., Bell, R. A., Hesser, J. E., Smith, G. H.: \n 1994, {\\it Can. J. Phys.} {\\bf 72}, 772.\n\\item Buonanno, R., Buzzoni, A., Corsi, C. E., Fusi-Pecci, F., Sandage, A. R.:\n 1986, \\SAIT 57 391... |
astro-ph0001019 | The Ulysses Supplement to the GRANAT/WATCH Catalog of Cosmic Gamma-Ray Bursts | [
{
"author": "K. Hurley"
}
] | We present 3rd interplanetary network (IPN) localization data for 56 gamma-ray bursts in the GRANAT/ WATCH catalog which occurred between 1990 November and 1994 September. These localizations are obtained by triangulation using various combinations of spacecraft in the IPN, which consisted of Ulysses , BATSE, Pioneer V... | [
{
"name": "ms.TEX",
"string": "%\\documentclass{aastex}\n\\documentstyle[12pt,aasms4]{article}\n\n\\begin{document}\n\n\\title{The Ulysses Supplement to the GRANAT/WATCH Catalog\nof Cosmic Gamma-Ray Bursts}\n\n\n\\author{K. Hurley}\n\\affil{University of California, Berkeley, Space Sciences Laboratory,\nBer... | [] |
astro-ph0001020 | HST/WFPC2 observations of the core of KjPn 8 | [
{
"author": "Jos\\'e Alberto L\\'opez"
}
] | % Narrow-band images of the core of the extraordinary poly-polar planetary nebula KjPn 8 have been obtained with the WFPC2 camera on board the Hubble Space Telescope. Spasmodic bipolar ejections, in changing directions have occurred over thousands of years to create KjPn 8. The central star is finally revealed in these... | [
{
"name": "lopez.tex",
"string": "\n\\documentstyle[11pt,newpasp,twoside,epsfig,epsf]{article}\n\\markboth{L\\'opez et al.}{HST/WFPC2 observations of KjPn 8}\n\\pagestyle{myheadings}\n\\nofiles\n\n% Some definitions I use in these instructions.\n\n\\def\\emphasize#1{{\\sl#1\\/}}\n\\def\\arg#1{{\\it#1\\/}}\n... | [] |
astro-ph0001021 | Testing envelope models of young stellar objects with submillimeter continuum and molecular-line observations | [
{
"author": "Michiel R. Hogerheijde\\altaffilmark{1}"
}
] | Theoretical models of star formation make predictions about the density and velocity structure of the envelopes surrounding isolated, low-mass young stars. This paper tests such models through high quality submillimeter continuum imaging of four embedded young stellar objects in Taurus and previously obtained molecular... | [
{
"name": "scuba.tex",
"string": "\\documentclass[preprint]{aastex}\n\n% Revised version including comments of referee; 7 December 1999.\n\n\\shorttitle{Testing YSO envelope models with continuum and line \nobservations}\n\\shortauthors{Hogerheijde \\& Sandell}\n\\begin{document}\n\n\\title{Testing envelope... | [
{
"name": "astro-ph0001021.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[Adams, Lada, \\& Shu(1987)]{adams:ysosed}\n{Adams}, F.~C., {Lada}, C.~J., \\& {Shu}, F.~H. 1987,\n\\newblock \\apj, 312, 788\n\n\\bibitem[Adams \\& Shu(1985)]{adams:irsed}\n{Adams}, F.~C. \\& {Shu}, F.~H. 1985,\n\\... |
astro-ph0001022 | A multipole-Taylor expansion for the potential \\ of gravitational lens MG~J0414+0534 | [] | We employ a multipole-Taylor expansion to investigate how tightly the gravitational potential of the quadruple-image lens MG~J0414+0534 is constrained by recent VLBI observations. These observations revealed that each of the four images of the background radio source contains four distinct components, thereby providing... | [
{
"name": "ms.tex",
"string": "% $ $Id: paper.tex,v 1.10 1999/12/15 21:44:40 cst Exp $\n%\\documentstyle[12pt,aasms4]{article}\n\\documentstyle[11pt,aaspp4]{article}\n%\\documentstyle[aas2pp4]{article}\n%\\documentstyle[11pt,eqsecnum,aaspp4]{article}\n%\\documentstyle[12pt,amssym,aasms4]{article}\n\n%\\rece... | [
{
"name": "astro-ph0001022.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[Angonin-Willaime et al. 1994]{angonin}\n Angonin-Willaime, M.-C., Vanderriest, C., Hammer, F. \\& Magain, M.\n 1994, A\\&A, 281, 388-394.\n\\bibitem[Chae, Khersonksy \\& Turnshek 1998]{model3}\n Chae, K.-H., ... |
astro-ph0001023 | Studies of Low-Mass Star Formation with ALMA | [
{
"author": "Neal J. Evans II"
}
] | ALMA will revolutionize the study of star formation by providing a combination of angular resolution and sensitivity that far exceeds that of present instruments. I will focus on studies of relatively isolated cores that are forming low-mass stars. There is a general paradigm for the formation of such stars, and there ... | [
{
"name": "evansn.tex",
"string": "%\n% Keywords: star formation, dust continuum emission, molecular line emission,\n% temperature, density, velocity\n%\n%\\documentstyle[11pt,newpasp,twoside,psfig]{article}\n\\documentstyle[11pt,newpasp,twoside,epsf]{article}\n\\markboth{Neal J. Evans II}{Studies of Low-Ma... | [] |
astro-ph0001024 | PHYSICAL CONDITIONS, GRAIN TEMPERATURES, AND ENHANCED VERY SMALL GRAINS IN THE BARNARD LOOP | [
{
"author": "Carl Heiles"
}
] | We derive the radio spectral index of the Barnard Loop (BL) from large-scale radio surveys at four frequencies and find it to be a thermal source. We use the radio data together with H$\alpha$ data to determine the electron temperature in BL, the $\lambda$ Ori HII region, and a high-latitude filament; all of these regi... | [
{
"name": "ms.tex",
"string": "%\\documentstyle[12pt,aasms4]{article}\n\\documentstyle[11pt,psfig,aaspp4]{article}\n\n\\begin{document}\n\n\\title{ PHYSICAL CONDITIONS, GRAIN TEMPERATURES, AND ENHANCED VERY SMALL\nGRAINS IN THE BARNARD LOOP}\n\n\\author{Carl Heiles}\n\\affil{Astronomy Department, University... | [] |
astro-ph0001025 | Resonant capture, counter-rotating disks, and polar rings | [
{
"author": "Scott Tremaine and Qingjuan Yu"
},
{
"author": "Peyton Hall"
},
{
"author": "Princeton"
},
{
"author": "NJ~08544-1001"
},
{
"author": "USA"
}
] | We suggest that polar rings and/or counter-rotating disks in flattened galaxies can be formed from stars captured at the Binney resonance, where the rate of precession of the angular momentum vector of a disk star equals the pattern speed of a triaxial halo. If the halo pattern speed is initially retrograde and slowly ... | [
{
"name": "flip.tex",
"string": "%\\documentstyle[referee,epsfig]{mn}\n\\documentstyle[onecolumn,epsfig]{mn}\n%\\documentstyle[epsfig]{mn}\n\\newif\\ifAMStwofonts\n%\\AMStwofontstrue\n%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n\\topmargin -1.8cm\n\\ifoldfss\n %\n \\newcommand{\\rmn}[1] {{\\rm #1}}\... | [
{
"name": "astro-ph0001025.extracted_bib",
"string": "\\begin{thebibliography}{99}\n\n\\bibitem[Bekki 1998]{bek98} Bekki K. 1998, ApJ 499, 635\n\n\\bibitem[Bertola, Buson \\& Zeilinger 1992]{ber92} Bertola F., Buson L. M., \\&\nZeilinger W. W. 1992, ApJ 401, L79\n\n\\bibitem[Bertola et al. 1996]{ber96} Bert... |
astro-ph0001026 | The Central X-Ray Point Source in Cassiopeia A | [
{
"author": "Deepto~Chakrabarty and Michael~J.~Pivovaroff"
}
] | The spectacular ``first light'' observation by the {\em Chandra X-Ray Observatory} revealed an X-ray point source near the center of the 300 yr old Cas~A supernova remnant. We present an analysis of the public X-ray spectral and timing data. No coherent pulsations were detected in the {\em Chandra}/HRC data. The 3$\sig... | [
{
"name": "casa.tex",
"string": "\\documentclass[preprint2]{aastex} % elec. submission version\n\n\\def\\ltsima{$\\; \\buildrel < \\over \\sim \\;$}\n\\def\\simlt{\\lower.5ex\\hbox{\\ltsima}}\n\\def\\gtsima{$\\; \\buildrel > \\over \\sim \\;$}\n\\def\\simgt{\\lower.5ex\\hbox{\\gtsima}}\n\n\\slugcomment{Subm... | [
{
"name": "astro-ph0001026.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\parskip=0pt\n\\parsep=0pt\n\\itemsep=0pt\n\n\\bibitem[Alcock \\& Illarionov 1980]{ai80}\nAlcock, C. \\& Illarionov 1980, ApJ, 235, 534\n\n\\bibitem[Alpar 1999]{alpar99}\nAlpar, A. 1999, preprint (astro-ph/9912228)\n\n\\bibit... |
astro-ph0001027 | Is Thermal Instability Significant in Turbulent Galactic Gas? | [
{
"author": "Enrique V\\'azquez-Semadeni$^1$"
},
{
"author": "Adriana Gazol$^2$ and John Scalo$^3$"
}
] | We investigate numerically the role of thermal instability (TI) as a generator of density structures in the interstellar medium (ISM), both by itself and in the context of a globally turbulent medium. We consider three sets of numerical simulations: {a)} flows in the presence of the instability only; {b)} flows in the ... | [
{
"name": "ms.tex",
"string": "%\\documentstyle{mn}\n%\\documentclass{mn}\n%\\documentstyle[12pt,aaspp4]{article}\n%\\documentstyle[12pt,aasms4]{article}\n\\documentstyle[aas2pp4]{article}\n%\\usepackage{graphics}\n\n\\def\\betiips1{\\beta_{i,i+1}}\n\\def\\gamef{{\\gamma^{\\rm e}}}\n\\def\\gamiips1{{{\\gamm... | [
{
"name": "astro-ph0001027.extracted_bib",
"string": "\\begin{thebibliography}{99}\n\n\\bibitem[]{Allen}Allen, S.W. \\& Fabian, A.C. 1998, MNRAS, 297, 57\n\n\\bibitem[]{balbus}Balbus, S.A., \\& Soker, N. 1989, ApJ, 341, 611\n\n\\bibitem[BVS99]{BVS99} Ballesteros-Paredes, J., V\\'azquez-Semadeni, E.,\n\\& Sc... |
astro-ph0001028 | The variability analysis of PKS 2155-304 | [
{
"author": "J.H. Fan\\inst{1,2}"
},
{
"author": "R.G. Lin\\inst{1}"
}
] | In this paper, the post-1977 photometric observations of PKS 2155-304 are compiled and used to discuss the variation periodicity. Largest amplitude variations ( $\Delta U = 1^{m}.5$; $\Delta B = 1^{m}.65$; $\Delta V = 1^{m}.85 $; $\Delta R = 1^{m}.25$; $\Delta I = 1^{m}.14 $) and color indices ( $(B-V) = 0.30\pm 0.06$;... | [
{
"name": "fan2155.tex",
"string": "\\documentstyle[11pt,aasms4]{article}\n\\begin{document}\n\n%\\documentstyle{l-aa}\n%\\begin{document}\n\n\n\\title{The variability analysis of PKS 2155-304}\n\n\n%\\author{J.H. Fan\\inst{1,2} \\and R.G. Lin\\inst{1}}\n%\\institute{ Center for Astrophysics, Guangzhou Norm... | [
{
"name": "astro-ph0001028.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem[]{} Bertaud CH., Wlerick G., V$\\acute{e}$ron P., et al. 1973,\nA\\&AS 11, 77\n\\bibitem[]{} Bowyer S., Brodie J., Clarke J. T., Henry J.P. 1984, ApJ 278, L103\n\\bibitem[]{} Brindle C., Hough J.H., Bailey J.A., et ... |
astro-ph0001029 | Long-term Variability Properties and Periodicity Analysis for Blazars | [
{
"author": "J.H. Fan"
}
] | In this paper, the compiled long-term optical and infrared measurements of some blazars are used to analysis the variation properties and the optical data are used to search for periodicity evidence in the lightcurve by means of the Jurkevich technique and the discrete correlation function (DCF) method. Some explanatio... | [
{
"name": "astro-ph0001029.tex",
"string": "\\documentstyle[11pt,aasms4]{article}\n\\begin{document}\n\n\\title{Long-term Variability Properties and \nPeriodicity Analysis for Blazars}\n\n\\author{J.H. Fan}\n\n\n\\affil{\n1. Center for Astrophysics, Guangzhou Normal University, Guangzhou 510400,\n China, e-... | [
{
"name": "astro-ph0001029.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem[]{} Abraham, Z. \\& Romero, G.E. 1999, A\\&A, 344, 61, 1999\n\\bibitem[]{} Angione, R.J. et al., 1981, AJ, 86, 653\n\\bibitem[]{} Angione, R.J. \\& Smith, H.J. 1985, AJ, 90, 2474\n\\bibitem[]{} Babadzhanyants, M.K. \... |
astro-ph0001030 | A Hard Medium Survey with ASCA.III.: a Type 2 AGN revealed from X-ray spectroscopy \thanks{Based on observations performed at the European Southern Observatory, Paranal, Chile} | [
{
"author": "R. Della Ceca \\inst{1}"
},
{
"author": "T. Maccacaro \\inst{1}"
},
{
"author": "P. Rosati \\inst{2} and V. Braito \\inst{1}"
}
] | In this paper we report the discovery of an hard X-ray selected Type 2 Seyfert galaxy and we present and discuss its X-ray and optical spectrum together with the radio to X-ray energy distribution. The X-ray source - AXJ2254+1146 - is part of the ASCA Hard Serendipitous Survey (HSS). % of Della Ceca et al. What makes t... | [
{
"name": "AA9395.tex",
"string": "%\\documentclass[referee]{aa}\n\\documentclass{aa}\n\\usepackage{psfig,latexsym,longtable}\n\n\\begin{document} \n\n\\thesaurus{03(13.25.2;11.19.1;12.03.3)}\n\n\\title{A Hard Medium Survey with ASCA.III.: a Type 2 AGN revealed from X-ray spectroscopy\n\\thanks{Based on obs... | [
{
"name": "astro-ph0001030.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n%\\bibitem[]{} Almaini, O., Shanks, T., Boyle, B.J., Griffiths, R.E., Roche, N., Stewart, G.C., and Georgantopoulos, I., 1996, MNRAS, 282, 295.\n\\bibitem[]{} Akiyama, M., et al., 1998a, astro-ph/9811012\n\\bibitem[]{} Akiya... |
astro-ph0001031 | Multiple Outflows in AFGL~2688 | [
{
"author": "Robert Lucas"
}
] | We present high resolution ($1\farcs 1 \times 0\farcs9$) imaging of the proto-planetary nebula AFGL 2688 in the CO (J=2--1) line using the IRAM interferometer. The observations reveal with unprecedented detail the structure and the kinematics of the gas ejected by the star over the past few hundred years and exemplify ... | [
{
"name": "rlucas-crl2688.tex",
"string": "\\documentstyle[11pt,newpasp,twoside,epsf]{article}\n\\markboth{R. Lucas, P. Cox \\& P.J. Huggins}{Multiple Outflows in the Egg Nebula}\n\\pagestyle{myheadings}\n\\nofiles\n\n% Some definitions I use in these instructions.\n\\newcommand {\\kms}{\\mbox{\\,km\\,s$^{-... | [] |
astro-ph0001032 | Limits on the Spatial Extent of AGN Measured with the Fine Guidance Sensors of the HST\footnote[1]{Based on observations made with the NASA/ESA {\em Hubble Space Telescope}, obtained from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under N... | [
{
"author": "Richard N. Hook"
}
] | The optical structure of several AGN has been studied using the Fine Guidance Sensors (FGS) on the Hubble Space Telescope (HST). The FGSs are interferometric devices which can resolve structure on scales of 20 milliarcsecs or less and hence have the potential to improve on the resolution attainable by HST's cameras. Th... | [
{
"name": "fgs-agn.tex",
"string": "\\documentstyle[12pt,aasms4]{article}\n\\begin{document}\n\n\\title {Limits on the Spatial Extent of AGN Measured \nwith the Fine Guidance Sensors of the HST\\footnote[1]{Based\non observations made with the NASA/ESA {\\em Hubble Space Telescope},\nobtained from the Space... | [] |
astro-ph0001033 | RADIO EMISSION OF THE GALACTIC X-RAYS BINARIES WITH RELATIVISTIC JETS | [
{
"author": "Sergei A. Trushkin"
},
{
"author": "{Special Astrophysical Observatory of Russian Academy of Sciences}"
},
{
"author": "{357147 Karachaevo-Cherkesia, Nizhnij Arkhyz, Russia }"
}
] | Variable non-thermal radio emission from Galactic X-ray binaries is a trace of relativistic jets, created near accretion disks. The spectral characteristics of a lot of radio flares in the X-ray binaries with jets (RJXB) is discussed in this report. We carried out several long daily monitoring programs with the RATAN-6... | [
{
"name": "gmic99.tex",
"string": "% from ----------------------------------- satr@cats.sao.ru\n\\documentstyle[12pt,psfig]{article}\n\\textwidth=17cm\n\\textheight=24cm\n\\voffset=-1.5cm\n\\oddsidemargin= -2.4mm\n\\evensidemargin= -2.4mm\n\\topmargin= -5.4mm\n\\headheight=12pt % 4.2mm\n\\headsep=32pt % ... | [
{
"name": "astro-ph0001033.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem{BT}\nBursov N.N., Trushkin S.A. 1995,\nMultifrequency observations of a recent radio flare in SS433.\nPis'ma in Astron. Zh., 21, pp.163-167.\n\n\\bibitem{F0}\nFender R.P., Burnell S.J.B., Waltman, E.B., 1997,\nThe ra... |
astro-ph0001034 | First Light Measurements of Capella with the Low Energy Transmission Grating Spectrometer aboard the Chandra X-ray Observatory | [
{
"author": "A.C.~Brinkman"
},
{
"author": "C.J.T.~Gunsing"
},
{
"author": "J.S.~Kaastra"
},
{
"author": "R.L.J.~van~der~Meer"
},
{
"author": "R.~Mewe"
},
{
"author": "F.~Paerels \\altaffilmark{1}"
},
{
"author": "A.J.J.~Raassen \\altaffilmark{2}"
},
{
"au... | We present the first X-ray spectrum obtained by the Low Energy Transmission Grating Spectrometer (LETGS) aboard the Chandra X-ray Observatory. The spectrum is of Capella and covers a wavelength range of 5--175~\AA\ (2.5--0.07~keV). The measured wavelength resolution, which is in good agreement with ground calibration, ... | [
{
"name": "apj_letter.tex",
"string": "%% Beginning of file 'revised_capella_draft.tex'\n%%\n%% This is a manuscript marked up using the\n%% AASTeX v5.0 LaTeX 2e macros.\n\n% \\documentclass{aastex}\n\n%% preprint produces a one-column, single-spaced document:\n\n \\documentclass[preprint]{aastex}\n\n%% pre... | [
{
"name": "astro-ph0001034.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem[Acton et al.(1972)]{Act72} Acton,~L.~W., Catura,~R.~C., \n\tMeyerott,~A., \\& Wolfson,~C.~J. 1972, Solar Phys., 26, 183\n\\bibitem[Bhatia \\& Doschek(1992)]{Bha92} Bhatia,~A.~K. \\& Doschek,~G.~A. 1992, \n\tAt. Data ... |
astro-ph0001035 | O-bearing Molecules in Carbon-rich Proto-Planetary Objects\footnotemark[1] | [
{
"author": "F. Herpin\\footnotemark[2]"
},
{
"author": "J. Cernicharo"
}
] | We present ISO LWS observations of the proto-planetary nebula CRL 618, a star evolving very fast to the planetary nebula stage. In addition to the lines of \COd, \COt, HCN and HNC, we report on the detection of \water and OH emission together with the fine structure lines of [OI] at 63 and 145 $\mu$m. The abundance of ... | [
{
"name": "reflastpaper.tex",
"string": "%\\documentclass []{aa}\n%\\usepackage {psfig,epsfig}\n%\\topmargin 2.cm\n%\\documentstyle[astroref-dbj,emulatedapj-dbj,psfig,epsfig]{article}\n\\documentstyle[12pt,aasms4,psfig,epsfig]{article}\n%\\voffset=-5mm\n%\\voffset=-25mm\n\n%\\input grafix\n%\\input grafix\n... | [] |
astro-ph0001037 | [
{
"author": "% %Begin Author names A. Comastri$^1$"
},
{
"author": "F. Fiore$^{2,3,4}$"
},
{
"author": "C. Vignali$^{1,5}$"
},
{
"author": "F. La Franca$^6$"
},
{
"author": "G. Matt$^6$"
}
] | The integrated emission of highly obscured AGN is expected to provide a major contribution to the X--ray energy density in the Universe: the X--ray background (XRB). The study of these objects is possible only at energies where the effects of absorption are less severe. For this reason we have carried out the {BeppoSAX... | [
{
"name": "comastri.tex",
"string": "\\documentstyle[psfig,epsf,conf-X]{article}\n%\n\\begin{document} \n\\small\n%\n\\def\\cgs{ ${\\rm erg~cm}^{-2}~{\\rm s}^{-1}$ } \n%\n\\heading{%\n%Begin Heading\n%\nThe BeppoSAX High Energy Large Area Survey (HELLAS): a progress report\n% End Heading\n}\n\\par\\medskip\... | [
{
"name": "astro-ph0001037.extracted_bib",
"string": "\\bibitem{Ak00} Akiyama M., et al., 2000, \\apj in press\n\n\\bibitem{B97} Boella G., et al., 1997, A\\&AS 122, 299 \n\n\\bibitem{C98} Cagnoni I., Della Ceca R., Maccacaro T., 1998, \\apj 493, 54 \n\n\\bibitem{C95} Comastri A., et al., 1995, \\aeta 296,... | |
astro-ph0001038 | [
{
"author": "% %Begin Author names R.Valdarnini$^{1}$"
},
{
"author": "S. Ghizzardi$^{2,4}$"
},
{
"author": "S. Bonometto$^{3,4}$ %End Author names"
}
] | A large set of TREESPH simulations is used to test the global morphology of galaxy clusters and its evolution against X--ray data. A powerful method to investigate substructures in galaxy clusters are the {power ratios} introduced by Buote $\&$ Tsai. We consider three flat cosmological models: CDM, \L~($\Omega_\Lambda ... | [
{
"name": "Valda.tex",
"string": "\\documentstyle[psfig,epsf,conf-X,10pt]{article}\n\\def\\etal{{\\rm et al.~}}\n\\def\\eg{{\\rm e.g.}}\n\\def\\ie{{\\rm i.e.}}\n\\def\\sub{{substructures}}\n\\def\\apim{{$\\Pi^{(m)}$}}\n\\def\\api2{{$\\Pi^{(2)}$}}\n\\def\\api3{{$\\Pi^{(3)}$}}\n\\def\\api4{{$\\Pi^{(4)}$}}\n\\... | [
{
"name": "astro-ph0001038.extracted_bib",
"string": "\\bibitem{bor93}\nB\\\"ohringer, H., 1993, eds. Silk, J., Vittorio, N., Proc. E.Fermi Summer \nSchool, Galaxy Formation \n\n\n\\bibitem{BT95}\nBuote D.A., Tsai J.C., 1995, ApJ, 452, 522\n\n\n\\bibitem{BT96}\nBuote D.A., Tsai J.C., 1996, ApJ, 458, 27\n\n\... | |
astro-ph0001039 | Antikaon condensation in neutron stars | [
{
"author": "Subrata Pal$^1$"
},
{
"author": "Debades Bandyopadhyay$^2$ and Walter Greiner$^1$"
}
] | We investigate the condensation of charged $K^-$ meson and neutral $\bar K^0$ meson in dense neutron star matter. Calculations are performed in relativistic mean field models in which both the baryon-baryon and (anti)kaon-baryon interactions are mediated by meson exchange. It is found that $\bar K^0$ condensation is qu... | [
{
"name": "kaonweb.tex",
"string": "\\documentstyle[preprint,prc,aps,epsfig]{revtex}\n\\tighten\n\\begin{document}\n\\draft\n%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n\\title{Antikaon condensation in neutron stars}\n\\author{Subrata Pal$^1$, Debades Bandyopadhyay$^2$ and Walter G... | [
{
"name": "astro-ph0001039.extracted_bib",
"string": "\\begin{thebibliography}{99}\n\n\\bibitem{Li} G.Q. Li, C.-H. Lee and G.E. Brown, Phys. Rev. Lett. \n79 (1997) 5214; Nucl. Phys. A625 (1997) 372.\n\\bibitem{Bet} H.A. Bethe and G.E. Brown, Sci. Am. 252 (1985) 60. \n\\bibitem{Pra97} M. Prakash, I. Bombaci,... |
astro-ph0001040 | Updated Information on the Local Group | [
{
"author": "Sidney van den Bergh"
}
] | The present note updates the information published in my recent monograph on \underline{The Galaxies of the Local Group}. Highlights include (1) the addition of the newly discovered Cetus dwarf spheroidal as a certain member of the Local Group, (2) an improved distance for SagDIG, which now places this object very clos... | [
{
"name": "paper.tex",
"string": "\\documentstyle[12pt,aaspp4]{article}\n\n\\newcommand{\\msun} {{{\\rm\\ M}_{\\sun}}}\n\n\\begin{document}\n\n\\title{Updated Information on the Local Group}\n\\author{Sidney van den Bergh}\n\\affil{\nDominion Astrophysical Observatory \\\\\nNational Research Council of Cana... | [] |
astro-ph0001041 | [] | [
{
"name": "Science2.tex",
"string": "\\documentstyle[11pt,flushrt,epsfig]{article}\n%\\documentstyle[11pt,epsfig]{article}\n\\def\\baselinestretch{2}\n\\textwidth=6.5in\n\\textheight=8.4in\n\\topmargin=0in\n\\headheight=0.15in\n\\oddsidemargin=0in\n\\evensidemargin=0in\n\\parindent=2em\n\\parskip=1.5ex\n\\n... | [
{
"name": "astro-ph0001041.extracted_bib",
"string": "\\begin{thebibliography}{99}\n%\\bibitem{hubble}\n\\noindent\n(1) E.P. Hubble, \n{\\it Proc. Natl. Acad. Sci. USA} {\\bf 15}, 168 (1929).\\\\ \n%\\bibitem{jim93} \n\\noindent\n(2) P.J.E. Peebles, {\\it Principles\nof Physical Cosmology}, pp. 340-342 \n(P... | ||
astro-ph0001042 | Eccentric stellar discs with strong density cusps and separable potentials | [
{
"author": "P.O. Box 45195-159"
},
{
"author": "Gava Zang"
},
{
"author": "Zanjan"
},
{
"author": "IRAN"
}
] | We introduce a class of eccentric discs with ``strong" density cusps whose potentials are of St\"ackel form in elliptic coordinates. Our models exhibit some striking features: sufficiently close to the location of the cusp, the potential and surface density distribution diverge as $\Phi \propto r^{-1}$ and $\Sigma \pro... | [
{
"name": "paperJR.tex",
"string": "%\\documentstyle[11pt]{article}\n%\\documentstyle[apjpt4]{article}\n\\documentstyle[epsf]{mn}\n%\\textwidth= 16 cm\n%\\textheight= 9 in\n%\\topmargin= -2.0 cm\n%\\headheight=0.0 mm\n%\\oddsidemargin=0 cm\n%\\evensidemargin=0 cm\n%\\def\\thefootnote{}\n%\\renewcommand{\\ba... | [
{
"name": "astro-ph0001042.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem[R1]{BT87}Binney J., Tremaine S., 1987, Galactic Dynamics, Princeton\nUniversity Press, Princeton\n\\bibitem[R2]{dZ85}de Zeeuw P.T., 1985, MNRAS, 216, 273\n\\bibitem[R3]{GB85}Gerhard O.E., Binney J., 1985, MNRAS, 216,... |
astro-ph0001043 | Photometric Properties of 47 Clusters of Galaxies: \\ I. The Butcher-Oemler Effect | [
{
"author": "V. E. Margoniner \\altaffilmark {1,2} and R. R. de Carvalho \\altaffilmark {2}"
}
] | We present $gri$ CCD photometry of 44 Abell clusters and 4 cluster candidates. Twenty one clusters in our sample have spectroscopic redshifts. Fitting a relation between mean $g$, $r$ and $i$ magnitudes, and redshift for this subsample, we have calculated photometric redshifts for the remainder with an estimated accura... | [
{
"name": "Margoniner.tex",
"string": "\\documentstyle[11pt,aaspp4]{article}\n\\def\\gtsim{\\hbox{\\raise.5ex\\hbox{$>$}\\llap{\\lower.5ex\\hbox{$\\sim$}}}}\n\\def\\ltsim{\\hbox{\\raise.5ex\\hbox{$<$}\\llap{\\lower.5ex\\hbox{$\\sim$}}}}\n\n\\begin{document}\n\n\\title{Photometric Properties of 47 Clusters o... | [] |
astro-ph0001044 | Interferometric $^{12}$CO Observations of the Central Disk of NGC 4631: An Energetic Molecular Outflow | [
{
"author": "Richard J. Rand"
}
] | We present interferometric observations of CO $J=1-0$ emission in the central regions of the edge-on galaxy NGC 4631, known for its extended gaseous halo and its tidal interactions. Previous single-dish observations revealed that almost all of the CO emission arises from a central ring or bar-like structure of length $... | [
{
"name": "n4631.tex",
"string": "% SAMPLE2.TEX -- AASTeX macro package tutorial paper.\n% The first item in a LaTeX file must be a \\documentstyle command to\n% declare the overall style of the paper. The \\documentstyle lines\n% that are relevant for the AASTeX macros are shown; one is uncommented out\n%... | [
{
"name": "astro-ph0001044.extracted_bib",
"string": "\\bibitem\n% command in the reference list below.\n%\n% Please see the AASTeX manual for a more complete discussion on how to make\n% \\cite-\n\\bibitem work for you. \n\n\\section{Introduction}\n\nNGC 4631 is one of the best examples of a nearby edge-... |
astro-ph0001045 | The Second Peak: The Dark-Energy Density and the Cosmic Microwave Background | [
{
"author": "Marc Kamionkowski and Ari Buchalter"
}
] | Supernova evidence for a negative-pressure dark energy (e.g., cosmological constant or quintessence) that contributes a fraction $\Omega_\Lambda\simeq0.7$ of closure density has been bolstered by the discrepancy between the total density, $\Omega_{tot}\simeq1$, suggested by the location of the first peak in the cosmic ... | [
{
"name": "second.tex",
"string": "% LaTeX file for ``The Second Peak: The Dark-Energy Density and the Cosmic\n% Microwave Background'' by Marc Kamionkowski and Ari Buchalter\n\\def\\hatn{{\\bf \\hat n}}\n\\def\\hatm{{\\bf \\hat m}}\n\\def\\hatnprime{{\\bf \\hat n'}}\n\\def\\hatnone{{\\bf \\hat n_1}}\n\... | [
{
"name": "astro-ph0001045.extracted_bib",
"string": "\\begin{thebibliography}{99}\n\n\\bibitem{CC} E.g., J. P. Ostriker and P. J. Steinhardt, {\\sl\n Nature} {\\bf 377}, 600 (1995); L. M. Krauss and\n M. S. Turner, {\\sl Gen. Rel. Grav.} {\\bf 27}, 1137 (1995);\n N. A. Bahcall et al., {\\sl Sci... |
astro-ph0001046 | NON-THERMAL EMISSION FROM RELATIVISTIC ELECTRONS IN CLUSTERS OF GALAXIES: A MERGER SHOCK ACCELERATION MODEL | [
{
"author": "Motokazu Takizawa"
}
] | We have investigated evolution of non-thermal emission from relativistic electrons accelerated at around the shock fronts during merger of clusters of galaxies. We estimate synchrotron radio emission and inverse Compton scattering of cosmic microwave background photons from extreme ultraviolet (EUV) to hard X-ray range... | [
{
"name": "ms.tex",
"string": "%\\documentstyle[12pt,aasms4]{article}\n%\\documentstyle[emulateapj,epsf]{article}\n\\documentstyle[12pt,aaspp4,epsf]{article}\n\\begin{document}\n%\\baselineskip=24pt\n%\\submitted{Accepted for publication in ApJ}\n\n\\title{NON-THERMAL EMISSION FROM RELATIVISTIC ELECTRONS IN... | [] |
astro-ph0001047 | Evidence for TeV gamma-ray emission from the shell type SNR RX\,J1713.7$-$3946 | [
{
"author": "H.~Muraishi\\inst{1}"
},
{
"author": "T.~Tanimori\\inst{2}"
},
{
"author": "S.~Yanagita\\inst{1}"
},
{
"author": "T.~Yoshida\\inst{1}"
},
{
"author": "M.~Moriya\\inst{2}"
},
{
"author": "T.~Kifune\\inst{3}"
},
{
"author": "S.~A.~Dazeley\\inst{4}"
},... | We report the results of TeV gamma-ray observations of the shell type SNR RX\,J1713.7$-$3946 (G347.3$-$0.5). The discovery of strong non-thermal X-ray emission from the northwest part of the remnant strongly suggests the existence of electrons with energies up to $\sim$ 100 TeV in the remnant, making the SNR a good can... | [
{
"name": "bm012.tex",
"string": "\\documentclass{aa}\n\\usepackage{graphics}\n\n\\begin{document}\n\\thesaurus{02 (08.19.5 RX\\,J1713.7-3946; 13.07.2)}\n\\title{Evidence for TeV gamma-ray emission from the shell type SNR\n RX\\,J1713.7$-$3946}\n\\author{H.~Muraishi\\inst{1},\nT.~Tanimori\\inst{2},\nS... | [
{
"name": "astro-ph0001047.extracted_bib",
"string": "\\begin{thebibliography}{}\n \\bibitem[1997]{allen97}\n Allen, G. E., et al., 1997,\n ApJ 487, L97\n \\bibitem[1987]{blandford87}\n Blandford, R. D. \\& Eichler, D., 1987,\n Phys. Rep. 154, 1\n \\bibitem[1998]{buckley98}\n Buc... |
astro-ph0001048 | The 24-Hour Night Shift:\\ Astronomy from Microlensing Monitoring Networks | [
{
"author": "Penny D. Sackett"
}
] | Scores of on-going microlensing events are now announced yearly by the microlensing discovery teams OGLE, MACHO and EROS. These early warning systems have allowed other international microlensing networks to focus considerable resources on intense photometric --- and occasionally spectroscopic --- monitoring of microle... | [
{
"name": "SackettBostonLens99.tex",
"string": "% Sackett contribution to proceedings of 1999 Boston Conference:\n% Gravitational Lensing: Recent Progress and Future Goals\n% Invited Targeted Talk:\n% The 24-Hour Night Shift: Astronomy from Microlensing Monitoring Networks\n% 28 July 1999, Boston, Massachus... | [] |
astro-ph0001049 | The Rise Times of High and Low Redshift Type Ia Supernovae are Consistent | [
{
"author": "Greg Aldering"
},
{
"author": "Robert Knop"
},
{
"author": "and Peter Nugent"
}
] | We present a self-consistent comparison of the rise times for low-- and high--redshift Type Ia supernovae. Following previous studies, the early light curve is modeled using a $t^2$ law, which is then mated with a modified Leibundgut template light curve. The best-fit $t^2$ law is determined for ensemble samples of low... | [
{
"name": "aldering.tex",
"string": "\\documentclass[preprint]{aastex}\n\\usepackage{psfig}\n\n\\begin{document}\n\n\\title{The Rise Times of High and Low Redshift Type Ia Supernovae\nare Consistent}\n\n\\author{Greg Aldering, Robert Knop, and Peter Nugent}\n\n\\affil{Lawrence Berkeley National Laboratory, ... | [
{
"name": "astro-ph0001049.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[Aguirre(1999)Aguirre]{aguirre_99}\nAguirre, A.~N. 1999, ApJ, 512, L19\n\n\\bibitem[Aldering(2000)Aldering]{aldering_nearby}\nAldering, G. 2000.\n\\newblock Type Ia Supernovae \\& Cosmic Acceleration.\n\\newblock In... |
astro-ph0001050 | Near-infrared emission-line galaxies in the Hubble Deep Field North | [
{
"author": "Fumihide {\\sc Iwamuro}"
},
{
"author": "Kentaro {\\sc Motohara}"
},
{
"author": "Toshinori {\\sc Maihara}"
},
{
"author": "Jun'ichi {\\sc Iwai}"
},
{
"author": "Hirohisa {\\sc Tanabe}"
},
{
"author": "Tomoyuki {\\sc Taguchi}"
},
{
"author": "Ryuji {\... | [
{
"name": "body.tex",
"string": "\\documentstyle[PASJadd]{PASJ95}\n\\input epsf.sty\n\n%\\draft\n\\markboth{}\n{}\n\\newcommand{\\vol}{}\n\\newcommand{\\no}{}\n\\newcommand{\\lett}{}\n\\newcommand{\\spage}{}\n\\newcommand{\\rdate}{1999 December 6}\n\\newcommand{\\adate}{2000 January 7}\n\\begin{document}\n\... | [] | |
astro-ph0001051 | Infrared Imaging of the Gravitational Lens PG~1115+080 with the Subaru Telescope | [
{
"author": "Fumihide {\\sc Iwamuro}"
},
{
"author": "$^1$ Kentaro {\\sc Motohara}"
},
{
"author": "$^1$ Toshinori {\\sc Maihara}"
},
{
"author": "$^1$ Jun'ichi {\\sc Iwai}"
},
{
"author": "$^1$"
},
{
"author": "Hirohisa {\\sc Tanabe}"
},
{
"author": "$^1$ Tomoyuk... | [
{
"name": "body.tex",
"string": "\\documentstyle[PASJadd]{PASJ95}\n\\input epsf.sty\n\n%\\draft\n\\markboth{}\n{}\n\\newcommand{\\vol}{}\n\\newcommand{\\no}{}\n\\newcommand{\\lett}{}\n\\newcommand{\\spage}{}\n\\newcommand{\\rdate}{1999 May 18}\n\\newcommand{\\adate}{1999 August 6}\n\\begin{document}\n\\titl... | [] | |
astro-ph0001052 | Near infrared imaging spectroscopy of NGC1275 | [
{
"author": "Alfred Krabbe\\inst{1,2}"
},
{
"author": "Bruce J.\\"
},
{
"author": "Sams\\inst{2} III"
},
{
"author": "Reinhard Genzel\\inst{2}"
},
{
"author": "Niranjan Thatte\\inst{2}"
},
{
"author": "Francisco Prada\\inst{3}"
}
] | We present H and K band imaging spectroscopy of the core regions of the cD/AGN galaxy NGC\,1275. The spectra, including lines from H{$_2$}, H, $^{12}\mbox{CO}$ bandheads, \mbox{[Fe\,{\sc ii}]}, and \mbox{[Fe\,{\sc iii}]}, are exploited to constrain the star formation and excitation mechanisms in the galaxy's nucleus. T... | [
{
"name": "n1275.tex",
"string": "%\\documentclass[referee]{aa}\n\\documentclass{aa}\n\\thesaurus{03(03.09.6; 11.01.2; 11.03.3; 11.09.1 NGC 1275; 13.09.1; 13.09.4)}\n\\usepackage{graphics}\n%\\usepackage{aabib99}\n\n%\\graphicspath{{:Figures_AA:}}\n%\\renewcommand{\\baselinestretch}{1.2}\n\\begin{document}\... | [
{
"name": "astro-ph0001052.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[1990]{Acosta-Pulido:90}\n{Acosta-Pulido} J.~A., {Perez-Fournon} I., {Calvani} M., {Wilson} A.~S., 1990,\n\\newblock {ApJ} {365}, 119\n\n\\bibitem[1978]{Beckwith:78}\n{Beckwith} S., {Persson} S.~E., {Neugebauer} G.,... |
astro-ph0001053 | Intracluster FIR emission as a tracer of cluster formation | [
{
"author": "Cristina C. Popescu \\inst{1,2}"
},
{
"author": "Richard J. Tuffs \\inst1"
},
{
"author": "J\\\"org Fischera \\inst1"
},
{
"author": "Heinrich V\\\"olk \\inst1"
}
] | We make predictions for the diffuse far-infrared (FIR) emission from dust in the intracluster medium (ICM) of the Virgo cluster using detailed information on potential dust sources, grain heating and sputtering rates available for this cluster from recent optical and X-ray studies. In the cluster core we identify the w... | [
{
"name": "eps.tex",
"string": "\n%-------------NEW ADDITIONS TO EXISTING ARTICLE.STY---------------------\n\n%\\catcode`\\@=11\n%\\long\\def\\@makefntext#1{ %\\parindent 1em\n%\\protect\\noindent \\hbox to 3.2pt {\\hskip-.9pt \n%$^{{\\ninerm\\@thefnmark}}$\\hfil}#1\\hfill} %can be used \n\n%\\def\\thefoot... | [
{
"name": "astro-ph0001053.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem{} Allen C.W., 1973, Astrophysical Quantities, third edn. Athlone,\nLondon \n\\bibitem{} Arimoto N., Yoshii Y., 1987, A$\\&$A 173, 23\n\\bibitem{} Arnaud K.A., Mushotzky R.F., 1998, ApJ 501, 119\n\\bibitem{} Bahcall J... |
astro-ph0001054 | The Hamburg/SAO Survey for Emission--Line Galaxies | [
{
"author": "U.~Hopp\\inst{1}\\fnmsep\\inst{9}"
},
{
"author": "D.~Engels\\inst{2}"
},
{
"author": "R.F.~Green\\inst{3}"
},
{
"author": "A.V.~Ugryumov\\inst{4}"
},
{
"author": "Y.I.~Izotov\\inst{5}\\fnmsep\\inst{10}"
},
{
"author": "H.-J.~Hagen\\inst{2}"
},
{
"aut... | We present the third list with results\footnote{ Tables 2 to 6 are available only in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html. Figures A1 to A9 will be made available only in the electronic version of the journal.} of the Hamburg/... | [
{
"name": "Hopp_Tab.tex",
"string": "%\\documentstyle[psfig]{aa}\n%\\pagestyle{empty}\n%\\renewcommand{\\baselinestretch}{1.3}\n\n%\\newcommand{\\MC}{\\multicolumn}\n%\\newcounter{qub}\n%\\setcounter{qub}{0}\n%\\newcommand{\\qq}{\\addtocounter{qub}{1}\\arabic{qub}}\n\n%\\begin{document}\n\n\\scriptsize\n\n\... | [
{
"name": "astro-ph0001054.extracted_bib",
"string": "\\begin{thebibliography}{99}\n\n\\bibitem[1981]{Baldwin81}\n Baldwin J.A., Phillips M.M., Terlevich R., 1981, PASP 93, 5\n\\bibitem[1994]{Coziol94}\n Coziol R., Demers S., Pena M., Barneoud R., 1994, AJ 108, 405C\n\\bibitem[1993]{Coziol93}\n Coziol R., D... |
astro-ph0001055 | The oxygen abundance deficiency in irregular galaxies | [
{
"author": "L.S. Pilyugin \\inst{1}"
},
{
"author": "F.Ferrini \\inst{2}"
}
] | The observed oxygen abundances in a number of irregular galaxies have been compared with predictions of the closed-box model of chemical and photometric evolution of galaxies. Oxygen is found to be deficient with respect to the predicted abundances. This is an indicator in favor of loss of heavy elements via galactic w... | [
{
"name": "9368.tex",
"string": "\\documentstyle{l-aa}\n\\begin{document}\n\n \\thesaurus{ 11 % Galaxies\n (11.01.1; % Galaxies:abundances\n 11.05.2; % Galaxies:evolution\n 11.09.4; % Galaxies:ISM\n 11.09.5) } % Galaxies:irregular\n... | [
{
"name": "astro-ph0001055.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\item {}\n Aparacio A., Gallart C., Bertelli G., 1997, AJ 114, 669\n\\item {}\n Bertelli G., Matteo M., Chiosi C., Bressan A., 1992, ApJ 388, 400\n\\item {}\n Bradamante F., Matteucci F., D'Ercole A., 1... |
astro-ph0001056 | On the Formation of Jets | [
{
"author": "Annalisa Celotti \\inst{1}"
},
{
"author": "Roger D. Blandford \\inst{2}"
}
] | The phenomenology of jets associated with a variety of black hole systems is summarized, emphasizing the constraints imposed on their origin. Models of jet formation are reviewed, focusing in particular on recent ideas concerning MHD models. Finally, the potential for advancing our understanding of jets both through fu... | [
{
"name": "acrdb.tex",
"string": "%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n% \"1readme\" Springer.\n% Please send the Tex and figure files and PS file \n%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n\\documentclass[runningheads]{cl2emult}\n\n\\usepackage{makeidx} ... | [
{
"name": "astro-ph0001056.extracted_bib",
"string": "\\begin{thebibliography}{7}\n\\addcontentsline{toc}{section}{References}\n\n\\bibitem{bbr} Begelman M.~C., Blandford R.~D., Rees M.~J. (1984) Rev. \nMod. Phys. {\\bf 56}, 255\n\n\\bibitem{burgarella} Burgarella D., Livio M., O'Dea C.~P. (Eds.) (1993)\nAs... |
astro-ph0001057 | On the origin of the luminosity - metallicity relation for late-type galaxies | [
{
"author": "L.S. Pilyugin \\inst{1}"
},
{
"author": "F.Ferrini \\inst{2}"
}
] | We consider the roles of two widely invoked mechanisms for the metallicity-luminosity correlation among late-type galaxies: higher astration level and decreasing efficiency of heavy-element loss with increasing luminosity. We find that both mechanisms contribute about equally to the range in oxygen abundance between lo... | [
{
"name": "9370.tex",
"string": "\\documentstyle{l-aa}\n\\begin{document}\n\n\n \\thesaurus{ 11 % Galaxies\n (11.01.1; % Galaxies:abundances\n 11.05.2; % Galaxies:evolution\n 11.09.4) } % Galaxies:ISM\n\n \\title{On the origin of the luminosity - ... | [
{
"name": "astro-ph0001057.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\item {}\n Bradamante F., Matteucci F., D'Ercole A., 1998, A\\&A 337, 338\n\\item {}\n de Young D., Gallagher J., 1990, ApJ 356, L15\n\\item {}\n de Young D., Heckman T., 1994, ApJ 431, 598\n\\item {}\n... |
astro-ph0001058 | Electron densities, temperatures and ionization rates in two interstellar clouds in front of $\beta$ Canis Majoris, as revealed by UV absorption lines observed with IMAPS | [
{
"author": "Edward B. Jenkins$^{1}$"
},
{
"author": "C\\'ecile Gry$^{2,3}$"
},
{
"author": "Olivier Dupin$^{3}$"
}
] | The spectrum of \bcma\ (Mirzam) between 1000 and 1200\AA\ was recorded at a wavelength resolving power $\lambda/\Delta\lambda\sim 60\,000$ by the Interstellar Medium Absorption Profile Spectrograph (IMAPS) during its orbital flight on the ORFEUS-SPAS~II mission in 1996. New information about interstellar absorption lin... | [
{
"name": "9228.tex",
"string": "\\documentclass[referee]{aa} % LaTeX A&A Monotype Times Fonts\n%\\documentclass[]{aa} % LaTeX A&A Monotype Times Fonts\n\\usepackage{psfig}\n\n\\newcommand{\\bcma}{$\\beta$~CMa}\n\\newcommand{\\acma}{$\\alpha$~CMa}\n\\newcommand{\\ecma}{$\\epsilon$~CMa}\n\\newcommand{\\v... | [
{
"name": "astro-ph0001058.extracted_bib",
"string": "\\begin{thebibliography}{}\n%\\bibitem{} Aldrovandi S.M.V., P\\'equignot D., 1973, A\\&A 25, 137\n\\bibitem{} Allan R.J., Clegg R.E.S., Dickinson A.S., Flower D.R., 1988,\nMNRAS, 235, 1245\n\\bibitem{} Anders E., Grevesse N., 1989, Geochim. Cosmochim. Ac... |
astro-ph0001060 | On the Interpretation of the Optical Spectra of L-type Dwarfs\thanks{ Based on observations made with the William Herschel Telescope (WHT) operated on the island of La Palma by the Isaac Newton Group at the Observatorio del Roque de los Muchachos of the Instituto de Astrof\'\i sica de Canarias; and on observations obta... | [
{
"author": "Ya. Pavlenko\\inst{1}"
},
{
"author": "M.\\"
},
{
"author": "R. Zapatero Osorio\\inst{2}"
},
{
"author": "R. Rebolo\\inst{2,3}"
}
] | We present synthetic optical spectra in the red and far-red (640--930\,nm) of a sample of field L dwarfs suitably selected to cover this new spectral class, and the brown dwarf GL\,229B. We have used the recent ``dusty'' atmospheres by Tsuji (\cite{tsuji00}) and by Allard (\cite{allard99}), and a synthesis code (Pavlen... | [
{
"name": "9324.tex",
"string": "\\documentclass{aa}\n%\\documentclass[referee]{aa}\n\n\\usepackage{graphics}\n\n\\begin{document}\n\n\\thesaurus{08 % Stars\n (08.01.03; % Stars: atmospheres\n 08.06.03; % Stars: fundamental parameters\n 08.12.02; % Stars: low-mass... | [
{
"name": "astro-ph0001060.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[1999]{allard99} Allard, F. 1999, private communication\n\n\\bibitem[1995]{allard95} Allard, F., Hauschildt, P. H. 1995, ApJ, 445, 433\n\n\\bibitem[1996]{allard96} Allard, F., Hauschildt, P. H., Baraffe, I., \n ... |
astro-ph0001061 | OBSERVATIONAL TESTS FOR THE COSMOLOGICAL PRINCIPLE AND WORLD MODELS | [
{
"author": "Ofer Lahav"
}
] | We review observational tests for the homogeneity of the Universe on large scales. Redshift and peculiar velocity surveys, radio sources, the X-Ray Background, the Lyman-$\alpha$ forest and the Cosmic Microwave Background are used to set constraints on inhomogeneous models and in particular on fractal-like models. Assu... | [
{
"name": "nato5.tex",
"string": "%5 Jan 2000 (OL), for astro-ph\n\n% The CRCKAPB.STY should be in your LaTeX directory.\n\n% Begin your text file with:\n\n\\documentstyle[NATO]{crckapb} \n\n\\input{psfig}\n\n\\def\\Mpc{\\, h^{-1} \\, {\\rm Mpc}}\n\\def\\bfw{ {\\bf w}}\n\n% Alternatives:\n% \\documentst... | [
{
"name": "astro-ph0001061.extracted_bib",
"string": "\\begin{thebibliography}{} % Note the empty braces!\n\n\n\n\n\\bibitem[]{}\nBaleisis, A., Lahav, O., Loan, A.J. \\& Wall, J.V. 1998, \nMNRAS, 297, 545\n\n\n\n\\bibitem[]{}\nBaugh C.M. \\& Efstathiou G. 1994, MNRAS , 267, 323\n\n\n\\bibitem[]{} \nBoldt, ... |
astro-ph0001062 | The Discovery of a Second Field Methane Brown Dwarf from Sloan Digital Sky Survey Commissioning Data\footnote{Based on observations obtained with the Sloan Digital Sky Survey and the Apache Point Observatory 3.5-meter telescope, which are owned and operated by the Astrophysical Research Consortium, and with the United ... | [
{
"author": "Zlatan I.\\ Tsvetanov\\altaffilmark{\\ref{JHU}}"
},
{
"author": "David A.\\ Golimowski\\altaffilmark{\\ref{JHU}}"
},
{
"author": "Wei Zheng\\altaffilmark{\\ref{JHU}}"
},
{
"author": "T.\\ R.\\ Geballe\\altaffilmark{\\ref{Gemini}}"
},
{
"author": "S.\\ K.\\ Leggett\\a... | We report the discovery of a second field methane brown dwarf from the commissioning data of the Sloan Digital Sky Survey (SDSS). The object, SDSS~J134646.45--003150.4 (SDSS~1346--00), was selected because of its very red color and stellar appearance. Its spectrum between 0.8--2.5~$\mu$m is dominated by strong absorpti... | [
{
"name": "sdss1346.tex",
"string": "%\\documentstyle[12pt,aasms4,flushrt]{article}\n\\documentstyle[11pt,aaspp4,flushrt]{article}\n\\def\\etal{{et al.}}\n\\def\\name{SDSS 1346-00}\n\\begin{document}\n\n\\title{The Discovery of a Second Field Methane Brown Dwarf from Sloan\nDigital Sky Survey Commissioning ... | [
{
"name": "astro-ph0001062.extracted_bib",
"string": "\\begin{thebibliography}{DUM}\n\\bibitem[Allard \\etal\\ 1996]{Allard96} Allard, F., Hauschildt, P.H.,\n Baraffe, I., \\& Chabrier, G. 1996, ApJ, 465, L123\n\\bibitem[Basri \\etal\\ 1996]{Basri96} Basri, G., Marcy, G. W., \\&\n Graham, J. R. 1996, Ap... |
astro-ph0001063 | The nature of RX~J0052.1-7319 | [
{
"author": "P. Kahabka\\inst{1}"
}
] | %______________________________________ Do not leave a blank line here! The nature of the X-ray source RX~J0052.1-7319 is discussed from observational data obtained from {\sl ROSAT} observations performed in 1995 and 1996. An accurate position is derived from {\sl ROSAT HRI} observations of the source performed in 1995... | [
{
"name": "9428.tex",
"string": "% laa.dem version 1 as of 23-Oct-90\n%\n% This is LAA.DEM, the demonstration file of the\n% LaTeX style file from Springer-Verlag for the\n% Astronomy and Astrophysics Main Journal\n%\n% It is for use with LaTeX version 2.09\n%\n% Please report all errors via e-mail to SPRIN... | [
{
"name": "astro-ph0001063.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem{} Corbet R.H.D., 1986, in: The Evolution of Galactic X-Ray Binaries,\n eds. J. Tr\\\"umper et al., Reidel Pub. Co., p. 63\n\\bibitem{} Cowley A.P., Schmidtke P.C., McGrath T.K., et al., 1997, PASP 109,\n ... |
astro-ph0001064 | Photometric modal discrimination in $\delta$ Scuti and $\gamma$~Doradus stars | [
{
"author": "Rafael Garrido"
}
] | The potential of photometric methods for the identification of $l$, the degree of spherical surface harmonic of a pulsating star, is investigated with special emphasis on Str\"omgren photometry applied to $\delta$ Scuti and $\gamma$ Dor variables. Limitations of actual model atmospheres when fine precision is required ... | [
{
"name": "rafag.tex",
"string": "% PSAMPLE2.TEX -- PASP Conference Proceedings macro package tutorial paper.\n% RAFAG.TEX\n\n%\\documentstyle[11pt,paspconf,epsf]{article}\n\\documentstyle[11pt,newpasp,twoside,epsfig]{article}\n\n\\markboth{Garrido, R.}{Photometric modal discrimination}\n\\setcounter{page}{... | [] |
astro-ph0001065 | The Angular Momentum Evolution of Very Low Mass Stars | [
{
"author": "Alison Sills"
},
{
"author": "M. H. Pinsonneault"
},
{
"author": "D. M. Terndrup"
}
] | We present theoretical models of the angular momentum evolution of very low mass stars (0.1 - 0.5 \Msunns). We also present models of solar analogues (0.6 - 1.1 \Msunns) for comparison with previous work. We investigate the effect of rotation on the effective temperature and luminosity of these stars. Rotation lowers t... | [
{
"name": "lowmass.pp.tex",
"string": "\\documentstyle[aaspp4,12pt]{article}\n\n\\newcommand{\\etal}{{\\em et~al. }}\n\\newcommand{\\Msun}{{M$_\\odot$ }}\n\\newcommand{\\Msunns}{{M$_\\odot$}}\n\\newcommand{\\vsini}{{$v\\sin i$ }}\n\\newcommand{\\vsinins}{{$v\\sin i$}}\n\\newcommand{\\wcrit}{{$\\omega_{crit}... | [] |
astro-ph0001066 | Generation of the Primordial Magnetic Fields during Cosmological Reionization | [
{
"author": "Nickolay Y.\\ Gnedin\\altaffilmark{1}"
},
{
"author": "Andrea Ferrara\\altaffilmark{2}"
},
{
"author": "and Ellen G.\\ Zweibel\\altaffilmark{3}"
}
] | We investigate the generation of magnetic field by the Biermann battery in cosmological ionization fronts, using new simulations of the reionization of the universe by stars in protogalaxies. Two mechanisms are primarily responsible for magnetogenesis: i) the breakout of I-fronts from protogalaxies, and ii) the propaga... | [
{
"name": "magfi.tex",
"string": "%Here's the file, and I hope we're converging. The main changes are:\n%\n%---small changes in language throughout, which I hope you agree make it read\n% more smoothly without suppressing anyone's personal style.\n%\n%---an estimate of the size of the fields created by th... | [] |
astro-ph0001067 | An asymmetric relativistic model for classical double radio sources | [
{
"author": "T.\\"
},
{
"author": "G.\\"
},
{
"author": "Arshakian\\thanks{On leave from Byurakan Astrophysical Observatory, Byurakan 378433, Armenia} and M.\\"
},
{
"author": "S.\\"
},
{
"author": "Longair"
},
{
"author": "Cavendish Astrophysics Group"
},
{
"auth... | There is substantial observational evidence against the symmetric relativistic model of FRII radio sources. An asymmetric relativistic model is proposed which takes account of both relativistic effects and intrinsic/environmental asymmetries to explain the structural asymmetries of their radio lobes. A key parameter of... | [
{
"name": "TigPaper1.tex",
"string": "\\documentstyle[epsfig]{mn}\n\n\\title[Asymmetric model for FRII sources]\n\t{An asymmetric relativistic model for classical double radio sources}\n \n\\author[T.\\,G.\\,Arshakian \\& M.\\,S.\\,Longair]\n {T.\\,G.\\,Arshakian\\thanks{On leave from Byurakan As... | [
{
"name": "astro-ph0001067.extracted_bib",
"string": "\\begin{thebibliography}{99}\n\\bibitem{} Akujor C.\\,E., Luedke E., Browne I.\\,W.\\,A., Leahy J.\\,P., Garrington S.\\,T., 1994, A\\&AS, 105, 247 (ALB)\n\\bibitem{} Akujor C.\\,E., Garrington S.\\,T., 1995, A\\&AS, 112, 235 (AG)\n\\bibitem{} Alexander ... |
astro-ph0001068 | On the peculiar red clump morphology in the open clusters NGC~752 and NGC~7789 | [
{
"author": "L\\'eo Girardi$^{1}$"
},
{
"author": "Jean-Claude Mermilliod$^2$"
},
{
"author": "Giovanni Carraro$^1$"
}
] | The red clump stars in the open cluster NGC~752 present a peculiar distribution in the colour-magnitude diagram (CMD): the clump is observed to present a faint extension, slightly to the blue of the main concentration of clump stars. We point out that a similar structure is present in the CMD of NGC~7789, and discuss t... | [
{
"name": "9256.tex",
"string": "\n% AA vers. 4.01, LaTeX class for Astronomy & Astrophysics\n% demonstration file\n% (c) Springer-Verlag HD\n%-----------------------------------------------------------------------\n\n%\\documentclass[referee]{aa} % for a refe... | [
{
"name": "astro-ph0001068.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem[1998]{bgdc} Bica E., Geisler D., Dottori H., Clari\\'a J.J., Piatti\n\tA.E., Santos Jr.\\ J.F.C., 1998, AJ 116, 723\n\\bibitem[1970]{rdc} Cannon R.D., 1970, MNRAS 150, 111\n\\bibitem[1994]{cc94} Carraro G., Chiosi C.... |
astro-ph0001069 | 2-D Radiation Transfer Model of Non-Spherically Symmetric Dust Shell in Proto-Planetary Nebulae | [
{
"author": "Kate Y.L. Su"
},
{
"author": "Volk"
},
{
"author": "K. and Kwok"
},
{
"author": "S."
}
] | %We present an 2-D radiative transfer model of non-spherically symmetric dust %shell. Assuming an axial symmetric dust evnelope with cavities %along the symmetric axis or a disk perpendicular to the axis, we have %applied the model to fit the spectral engery distribution (SED) and %the images of three proto-planetary n... | [
{
"name": "aspn-nonsp2.tex",
"string": "\\documentstyle[11pt,newpasp,twoside,epsf]{article}\n\\markboth{Su, Volk, \\& Kwok}{2-D model of PPN}\n\\pagestyle{myheadings}\n\\nofiles\n\n% Some definitions I use in these instructions.\n\n\\def\\emphasize#1{{\\sl#1\\/}}\n\\def\\arg#1{{\\it#1\\/}}\n\\let\\prog=\\ar... | [] |
astro-ph0001070 | [
{
"author": "F.H. Briggs"
}
] | [
{
"name": "fbriggs_mor99.tex",
"string": "\\documentstyle[12pt,moriond]{article}\n% This is a template file for the proceedings of the XIXth Moriond\n% Astrophysics Meeting ``Building Galaxies: from the Primordial Universe to the Present'', Les\n% Arcs, March 1999. \n%\n\\begin{document}\n%Here you should ... | [
{
"name": "astro-ph0001070.extracted_bib",
"string": "\\bibitem{bli99}Blitz, L., Spergel, D.~N., Teuben, \n P.~J., Hartmann, D., \\& Burton, W.~B. 1999, ApJ, 514, 818\n\n\\bibitem{bra99}Braun, R., \\& Burton, W.~B 1999, \n A\\&A, 341, 437 \n\n\\bibitem{bri99} Briggs, F.H. 1999, in Highly Redshifted Radi... | ||
astro-ph0001071 | % DISCOVERY OF A LOW SURFACE BRIGHTNESS OBJECT NEAR SEYFERT'S SEXTET | [
{
"author": "\\sc Takashi Murayama\\altaffilmark{1}"
},
{
"author": "Shingo Nishiura"
},
{
"author": "and Tohru Nagao\\altaffilmark{1}"
}
] | We report the discovery of a low surface brightness (LSB) object serendipitously found during deep CCD imaging of a compact group of galaxies, Seyfert's Sextet, in $V\!R$ and $I$ bands. The LSB object is located 2\farcm3 southwest from the group center. Its surface brightness within the angular effective radii of $r_{e... | [
{
"name": "ms.tex",
"string": "%\n% Murayama et al.\n%\n% Submitted version Dec. 4, 1999\n% Revised on Dec. 24, 1999\n% very minor revisions on Dec. 25, 1999\n\n%\\documentstyle[aasms4,12pt]{article}\n\\documentstyle[emulateapj]{article}\n\\newcommand{\\ts}{\\thinspace}\n\\begin{document}\n\n\\title{%\n... | [] |
astro-ph0001072 | The Stellar Population Histories of Local Early-Type Galaxies. I. Population Parameters | [
{
"author": "S. C. Trager\\altaffilmark{1}"
}
] | This paper commences a series of investigations into the stellar populations of local elliptical galaxies as determined from their integrated spectra. The goal of the series is to determine the star formation and chemical evolution histories of present-day elliptical galaxies. The primary galaxy sample analyzed is that... | [
{
"name": "paper1_accepted.tex",
"string": "\\documentclass{article}\n\\usepackage{emulateapj}\n\\usepackage{apjfonts}\n%\\usepackage{amssymb}\n\\usepackage[american]{babel}\n\n\\def\\phn{\\phantom{0}}\n\\def\\phd{\\phantom{.}}\n\\newcommand{\\kms}{\\ensuremath{\\mathrm{km\\ s^{-1}}}}\n\\newcommand{\\fe}{\\... | [
{
"name": "astro-ph0001072.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem[Arimoto 1996]{Arimoto96} Arimoto, N. 1996, in From Stars to\nGalaxies: The Impact of Stellar Physics on Galaxy Evolution, ed.\\\nC. Leitherer, U. Fritze-von Alvensleben, \\& J. Huchra, A. S. P. Conf.\\\nSer., vol.\\... |
astro-ph0001073 | \hangindent\abstractindent \hangafter 0 \relax | [
{
"author": "Maartje N. Sevenster \\inst{1,3}"
},
{
"author": "Herwig Dejonghe\\inst{2}"
},
{
"author": "Katrien Van Caelenberg\\inst{2}"
},
{
"author": "Harm J. Habing\\inst{1}"
}
] | We present dynamical distribution functions for a homogeneous sample of oxygen--rich, evolved, intermediate--mass stars in the inner galactic plane. We use an axisymmetric, two--component St\"ackel potential that satisfies recent constraints on the galactic potential, amongst others a slightly declining local rotation ... | [
{
"name": "9106.inputs.tex",
"string": "%% Macros for thesis table of contents\n\n\n\\font \\mnsbl=cmbx10 scaled\\magstep5 % Chapter\n\\font \\mnsbm=cmbx10 scaled\\magstep4 % Voorblad\n\\font \\mnsb=cmbx10 scaled\\magstep3 % Section\n\\font \\mnsbs=cmbx10 scaled\\magstep2 % Section\n\\font \\mnsi=cmr10 scal... | [
{
"name": "astro-ph0001073.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem{} Allen D., Hyland A., Jones T., 1983\\mnras 204 1145\n\n\\bibitem{} Batsleer P., Dejonghe H., 1994\\aa 287 43\n\\bibitem{} Batsleer P., Dejonghe H., 1995\\aa 294 693\n\n\\bibitem{} Binney J., Dehnen W., 1997\\mnra... |
astro-ph0001074 | SUPERNOVA REMNANTS, PULSARS AND THE INTERSTELLAR MEDIUM - SUMMARY OF A WORKSHOP HELD AT U SYDNEY, MARCH 1999 | [
{
"author": "Vikram Dwarkadas $^{1}$"
},
{
"author": "Lewis Ball $^{1}$"
},
{
"author": "James Caswell $^{2}$"
},
{
"author": "Anne Green $^{3}$"
},
{
"author": "Simon Johnston $^{1}$"
},
{
"author": "Brian Schmidt $^{4}$"
},
{
"author": "Mark Wardle $^{1}$"
}
] | and % | [
{
"name": "astro-ph0001074.tex",
"string": "%\n% LaTeX template file for\n% Publications of the Astronomical Society of Australia.\n% Version 2.4 - 28 April 1997\n%\n% The most current version of this file can be found at:\n% http://www.atnf.csiro.au/pasa/template\n%\n% Other information on Electronic PASA ... | [] |
astro-ph0001075 | The first galaxies: clues from element abundances | [
{
"author": "Max Pettini"
}
] | {} It has recently become possible to measure directly the abundances of several chemical elements in a variety of environments at redshifts up to $z \simeq 5$. In this review I summarise the latest observations of Lyman break galaxies, damped Lyman alpha systems and the Lyman alpha forest with a view to uncovering any... | [
{
"name": "mpettini.tex",
"string": "%%%%%%%%%%%%%%%\n\n% RSGUIDE.TEX %\n\n%%%%%%%%%%%%%%%\n\n\n\n% Guide to preparing TeX articles for Royal\n\n% Society articles using RSPUBLIC.CLS\n\n% Use this file as a test file\n\n\n\n\n\\documentclass{rspublic}\n\n\n\\usepackage{graphicx}\n\\usepackage{epsfig}\n\n\\d... | [
{
"name": "astro-ph0001075.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\item Centuri\\'{o}n, M., Bonifacio, P., Molaro, P., \\& Vladilo, G. 1998, ApJ, 509, 620\n\n\\item Cowie, L.L., \\& Songaila, A. 1998, Nature, 394, 44\n\n\\item Dav\\'{e}. R., Hellsten, U., Hernquist, L., Katz, N., \\& Wein... |
astro-ph0001076 | Cosmological SPH simulations with four million particles:\\ statistical properties of X-ray clusters in a low-density universe | [
{
"author": "Kohji Yoshikawa"
}
] | We present results from a series of cosmological SPH (smoothed particle hydrodynamics) simulations coupled with the P$^3$M (Particle--Particle--Particle--Mesh) solver for the gravitational force. The simulations are designed to predict the statistical properties of X-ray clusters of galaxies as well as to study the for... | [
{
"name": "clustsimu.tex",
"string": "%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n%\n% Cosmological SPH simulations with four million particles:\n% statistical properties of X-ray clusters in a low-density universe\n%\n% K.Yoshikawa, Y.P.Jing & Y.Suto\n... | [
{
"name": "astro-ph0001076.extracted_bib",
"string": "\\begin{thebibliography}{}\n%\\parskip=-1pt\n%\\baselineskip=14pt\n \\bibitem[Bertschinger(1995)]{Bertschinger1995} \n Bertschinger, E. 1995, astro-ph/9506070\n \\bibitem[Bryan \\& Norman(1998)]{Bryan1998} \n Bryan, G.L. \\& Norman, M.L. 1998, A... |
astro-ph0001077 | Neutron Star Mass Determinations | [
{
"author": "M.~H.~van Kerkwijk"
}
] | I review attempts made to determine the properties of neutron stars. The focus is on the maximum mass that a neutron star can have, or, conversely, the minimum mass required for the formation of a black hole. There appears to be only one neutron star for which there is strong evidence that its mass is above the canonic... | [
{
"name": "proceedings.tex",
"string": "%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n% This is a sample input file for your contribution to a multi-\n% author book to be published by Springer Verlag.\n%\n% Please use it as a template for your own input, and please\n% follow the instructi... | [
{
"name": "astro-ph0001077.extracted_bib",
"string": "\\begin{thebibliography}{99}\n%\n\\addcontentsline{toc}{section}{References}\n\n\\bibitem{bkvk+00}\n Barziv O., Kaper L., Van Kerkwijk M.~H., Telting J., Van Paradijs\n J., 2000, in preparation \n\\bibitem{bcc+97}\n Bildsten L., Chakrabarty D., Chiu J... |
astro-ph0001078 | Radiative Processes and Geometry of Spectral States of Black-hole Binaries | [
{
"author": "A. A. Zdziarski"
}
] | I review radiative processes responsible for X-ray emission in the hard (low) and soft (high) spectral states of black-hole binaries. The main process in the hard state appears to be thermal Comptonization (in a hot plasma) of blackbody photons emitted by a cold disk. This is supported by correlations between the spect... | [
{
"name": "zdziarski_v3.tex",
"string": "\\documentstyle[11pt,newpasp,twoside,epsf]{article}\n\n%version 16 Jan. 00\n\n\\markboth{Zdziarski}{Spectral States of Black-hole Binaries}\n\\pagestyle{myheadings}\n\\setcounter{page}{153}\n\n\\begin{document}\n\n\\title{Radiative Processes and Geometry of Spectral ... | [] |
astro-ph0001079 | Can DNA bases be produced during molecular cloud collapse? | [
{
"author": "Sonali Chakrabarti and Sandip K. Chakrabarti"
}
] | Using a reasonably large chemical reaction network consisting of $421$ species, we show that along with normal chemical evolution of molecular cloud during collapse and star formation, significant amount of adenine, a DNA base, may be produced after an evolution of $10^{6-7}$ years. This findings may shed light on whet... | [
{
"name": "rn.tex",
"string": "\\documentstyle[psfig,epsf]{l-aa}\n\\def\\lsim{\\lower.5ex\\hbox{$\\; \\buildrel < \\over \\sim \\;$}}\n\\def\\gsim{\\lower.5ex\\hbox{$\\; \\buildrel > \\over \\sim \\;$}}\n\\newcommand{\\eqb}{\\begin{eqnarray}}\n\\newcommand{\\eqe}{\\end{eqnarray}}\n\\newcommand{\\mdot}{\\sta... | [
{
"name": "astro-ph0001079.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\def\\ref#1\\par{\\parshape=2 0in 14.5cm 1cm 13.5cm {#1} \\par}\n\\parskip=0pt\n\\parindent=0pt\n\n\\bibitem[]{} Chandrasekhar S. 1939, An Introduction to Stellar Structure (Chicago: Univ. of Chicago Press)\n\\bibitem[]{} ... |
astro-ph0001080 | X-ray and optical observations of three clusters of galaxies: Abell 901, Abell 1437, and Abell 3570\thanks{Partly based on observations collected at the European Southern Observatory} | [
{
"author": "Sabine Schindler"
}
] | We analyse three clusters of galaxies, Abell 901 (z=0.17), Abell 1437 (z=0.13) and Abell 3570 (z=0.037). They have low to intermediate X-ray fluxes and an irregular morphology in the ROSAT All-Sky Survey (RASS). These clusters are chosen to test the abilities and limitations of the RASS in terms of cluster fluxes and c... | [
{
"name": "ds9209.tex",
"string": "%\\documentstyle[times]{l-aa}\n\\documentclass{aa}\n%\\documentclass[referee]{aa}\n%\\documentstyle{l-aa}\n%\\documentstyle[l-aa-fix]{l-aa}\n%\\documentstyle[l-aa-fix,referee]{l-aa}\n\\def\\msol{{M}_{\\odot}}\n\\def\\lsol{{L}_{\\odot}}\n\\def\\grsim{\\,\\lower 1mm \\hbox{\... | [
{
"name": "astro-ph0001080.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem{} Abell G.O., Corwin H.G., Olowin R.P., 1989, ApJS 70, 1\n\\bibitem{} Allen S.W., Fabian A.C., 1998, MNRAS 297, L57\n\\bibitem{} Arnaud M., Evrard A.E., 1999, MNRAS 305, 631\n\\bibitem{} Bender R., Moellenhof C., 198... |
astro-ph0001081 | A limit-cycle model for the binary supersoft X-ray source RX\,J0513.9-6951 | [
{
"author": "K. Reinsch \\inst{1}"
},
{
"author": "A. van Teeseling\\inst{1}"
},
{
"author": "A. R. King\\inst{2}"
},
{
"author": "K. Beuermann\\inst{1}"
}
] | We present new results of our X-ray monitoring of the transient binary supersoft X-ray source RX\,J0513.9--6951 in the LMC and of our re-analysis of optical light curves obtained during the MACHO project. We have covered a complete X-ray outburst cycle with the ROSAT HRI detector. From the amplitude and timescale of th... | [
{
"name": "b1292.tex",
"string": "%\\documentclass[referee]{aa} % for a referee version\n\\documentclass{aa}\n\\usepackage{psfig}\n\\usepackage{graphics}\n%\n\\newcommand{\\rxj}{RX\\,J0513}\n%\n\\begin{document}\n\n%\\special{!userdict begin /bop-hook{gsave 150 30 translate\n%0 rotate /Times-Roman findfont ... | [
{
"name": "astro-ph0001081.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem{ASL88} Adams F.C., Shu F.H., Lada C.J., 1988, ApJ 326, 865\n\\bibitem{Alcetal96} Alcock C., Allsman R.A., Alves D. et al., 1996, \n MNRAS 280, L49\n\\bibitem{Cowetal93} Cowley A.P., Schmidtke P.C., Hutchings J.B.... |
astro-ph0001082 | The dark matter distribution in disk galaxies | [
{
"author": "Annamaria Borriello$^1$ \\& Paolo Salucci$^1$"
},
{
"author": "(1) International School of Advanced Studies SISSA-ISAS -- Trieste"
},
{
"author": "I"
}
] | We use high--quality optical rotation curves of 9 low--luminosity disk galaxies to obtain the velocity profiles of the surrounding dark matter halos. We find that they increase linearly with radius at least out to the edge of the stellar disk, implying that, over the entire stellar region, the density of the dark halo ... | [
{
"name": "paper.tex",
"string": "\\documentstyle{mn}\n\\def\\lsim{\\, \\lower2truept\\hbox{${<\n\\atop\\hbox{\\raise4truept\\hbox{$\\sim$}}}$}\\,}\n\n\\def\\gsim{\\, \\lower2truept\\hbox{${>\n\\atop\\hbox{\\raise4truept\\hbox{$\\sim$}}}$}\\,}\n\n\\input psfig.tex\n\n\\title{The dark matter distribution in ... | [
{
"name": "astro-ph0001082.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[]{}\nBegeman, K.G., Broeils, A.H. \\& Sanders, R.H. (1991) MNRAS, {\\bf 249}, 523.\n\n\\bibitem[]{}\nBevington, P.R. \\& Robinson, D.K. (1992) {\\it Data reduction and error\nanalysis}; Boston: McGraw--Hill\n\n\\... |
astro-ph0001083 | Observation of Microlensing towards the Galactic Spiral Arms. {\sc EROS II} 3 year survey \thanks{This work is based on observations made at the European Southern Observatory, La Silla, Chile.} | [
{
"author": "{\\sc EROS} Collaboration"
}
] | We present an analysis of the light curves of 9.1 million stars observed during three seasons by {\sc EROS} (Exp\'erience de Recherche d'Objets Sombres), in the Galactic plane away from the bulge. Seven stars exhibit luminosity variations compatible with gravitational microlensing effects due to unseen objects. The cor... | [
{
"name": "bs3y.tex",
"string": "\\documentstyle[epsfig,twoside,rotating]{aa}\n%\\documentstyle[epsfig,twoside,draftcopy,rotating]{aa}\n%\\documentstyle[epsfig,twoside,referee,rotating]{aa}\n\\newcommand{\\Msol}{M_\\odot}\n\\newcommand{\\Rsol}{R_\\odot}\n\\newcommand{\\degree}{^\\circ}\n\\newcommand{\\gsct}... | [
{
"name": "astro-ph0001083.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem[Afonso {\\it et al.} 1999]{afonso}Afonso C., Alard C., Albert J.-N. {\\it et al.} ({\\sc EROS} Coll.), 1999, A\\&A 344, L63\n\\bibitem[Alcock {\\it et al.} 1993]{machlmc}Alcock C., Akerlof C.W., Allsman R.A. {\\it et... |
astro-ph0001084 | Signatures of galactic magnetic lensing\\ upon ultra high energy cosmic rays | [
{
"author": "Diego Harari$^a$"
},
{
"author": "Silvia Mollerach$^b$ and Esteban Roulet$^b$"
},
{
"author": "$^a$Departamento de F\\'\\i sica"
},
{
"author": "FCEyN"
},
{
"author": "Universidad de Buenos Aires"
},
{
"author": "Ciudad Universitaria - Pab. 1"
},
{
"a... | We analyse several implications of lensing by the regular component of the galactic magnetic field upon the observed properties of ultra high energy cosmic rays. Magnetic fields deflect cosmic ray trajectories, causing flux (de)magnification, formation of multiple images of a single source, and time delays. We derive t... | [
{
"name": "bgal2.tex",
"string": "\\documentclass[12pt]{JHEP}\n%\\documentclass[draft]{JHEP}\n\\usepackage{epsfig}\n\n\\def\\lsim{\\mathrel{\\mathpalette\\fun <}}\n\\def\\gsim{\\mathrel{\\mathpalette\\fun >}}\n\\def\\fun#1#2{\\lower3.6pt\\vbox{\\baselineskip0pt\\lineskip.9pt\n \\ialign{$\\mathsurround=0pt#... | [
{
"name": "astro-ph0001084.extracted_bib",
"string": "\\begin{thebibliography}{100}\n\n\\bibitem{sigl98}P. Bhattacharjee and G. Sigl, \n``Origin and propagation of extremely high-energy cosmic rays'',\n{\\it Phys. Rep.} (in press), \\astroph{9811011}. \n\n\\bibitem{I}D. Harari, S. Mollerach and E. Roulet,\n... |
astro-ph0001085 | The discovery of the optical/IR counterpart of the 12\,s transient X--ray pulsar \src\,\thanks{Partially based on observations carried out at ESO, La Silla, Chile (62.H--0513)} | [
{
"author": "G. L. Israel"
},
{
"author": "$^{1,}$\\thanks{Affiliated to ICRA.} S. Covino"
},
{
"author": "$^2$ S. Campana"
},
{
"author": "$^{2, \\dag~}$ V.F. Polcaro"
},
{
"author": "$^3$ P. Roche"
},
{
"author": "$^4$ L. Stella"
},
{
"author": "$^{1,\\dag}$ \\n... | We report the discovery of the optical counterpart of the 12.3\,s transient X--ray pulsar \src. We re--analysed archival \R PSPC observations of \src\, obtaining two new refined positions, $\sim$14\arcsec\ and $\sim$18\arcsec\ away from the previously published one, and a new spin period measurement. Based on these res... | [
{
"name": "GS0834_pap.tex",
"string": "%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% %\n\\documentstyle{mn}\n\\newcommand{\\Vol}[1]{{\\bf #1}}\n\\newcommand{\\ad}{$^o\\,$}\n\\newcommand{\\as}{$^{\\prime\\prime}~$}\n\\newcommand{\\am}{$^{\\prime}~$}\n\\newcommand{\\h}{$^{h}~~$}\n\\newcommand{\\m}{$^... | [
{
"name": "astro-ph0001085.extracted_bib",
"string": "\\begin{thebibliography}{} \n\\bibitem{ } Allen D., 1993, IRIS Users Manual, Anglo-Australian Observatory \nmanual 30a, version 2.5 \n\\bibitem{ } Aoki T., Dotani T., Ebisawa K., et al., 1992, PASJ, 44, 641 \n\\bibitem{ } Belloni T., Hasinger G., Pietsch... |
astro-ph0001086 | Fluorescent Excitation of Spectral Lines In Planetary Nebulae | [
{
"author": "Guo Xin Chen and Anil K. Pradhan"
}
] | Fluorescent excitation of spectral lines is demonstrated as a function of temperature-luminosity and the distance of the emitting region from the central stars of planetary nebulae. The electron densities and temperatures are determined, and the method is exemplified through a detailed analysis of spectral observations... | [
{
"name": "apjl.tex",
"string": "%%\n%% Beginning of file 'sample.tex'\n%%\n\n%\\documentclass{aastex}\n\n%% preprint produces a one-column, single-spaced document:\n\n% \\documentclass[preprint]{aastex}\n\n%% preprint2 produces a double-column, single-spaced document:\n\n\\documentclass[preprint2]{aastex}\... | [
{
"name": "astro-ph0001086.extracted_bib",
"string": "\\begin{thebibliography}{}\n\\bibitem[Ahern \\etal(1977)]{ahe77} Ahern, F.J., FitzGerald, M.F., Marsh, K.A., \\& Purton, C.R.,\n1977, A\\&A, 58, 35 \n\\bibitem[Aller \\etal(1985)]{all85} Aller, L.H., Keys, C.D., \\& Czyzak, S.J., 1985,\n... |
astro-ph0001087 | Testing population synthesis models with globular cluster colors | [
{
"author": "Pauline Barmby \\& John P. Huchra"
}
] | We have measured an extensive set of $UBVRIJHK$ colors for M31 globular clusters \citep{b00}. We compare the predicted simple stellar population colors of three population synthesis models to the intrinsic colors of Galactic and M31 globular clusters. The best-fitting models fit the cluster colors very well -- the weig... | [
{
"name": "BH_preprint.tex",
"string": "\\documentclass[preprint2]{aastex}\n\\newcommand{\\vi}{\\hbox{$V\\!-\\!I$}}\n\\newcommand{\\uv}{\\hbox{$U\\!-\\!V$}}\n\\newcommand{\\jk}{\\hbox{$J\\!-\\!K$}}\n\\newcommand{\\vk}{\\hbox{$V\\!-\\!K$}}\n\\newcommand{\\vh}{\\hbox{$V\\!-\\!H$}}\n\\newcommand{\\ubvri}{\\hbo... | [
{
"name": "astro-ph0001087.extracted_bib",
"string": "\\begin{thebibliography}{24}\n\\expandafter\\ifx\\csname natexlab\\endcsname\\relax\\def\\natexlab#1{#1}\\fi\n\n\\bibitem[{Barmby {et~al.}(2000)Barmby, Huchra, Brodie, Forbes, Schroder, \\&\n Grillmair}]{b00}\nBarmby, P., Huchra, J.~P., Brodie, J.~P., F... |
astro-ph0001088 | Evolution of Cluster Galaxies in Hierarchical Clustering Universes | [
{
"author": "Takashi {\\sc Okamoto} and Asao {\\sc Habe}"
}
] | [
{
"name": "paper.tex",
"string": "\\documentstyle[PASJadd,psfig]{PASJ95}\n%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n% PASJ LaTex example1\n%\n%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n%\\draft\n\n\\markboth{}\n{}\n\n\\newcommand{\\vol}{}\n\\newcommand{\\no}{}\n\\newcommand{\\lett}{}\n\\newcommand{\\spage}{}... | [] | |
astro-ph0001089 | Constraints on Cosmological Parameters from the Ly$\alpha$ Forest Power Spectrum and COBE-DMR | [
{
"author": "John Phillips$^{1}$"
},
{
"author": "David H. Weinberg$^{2}$"
},
{
"author": "\\linebreak Rupert A. C. Croft$^{2,3}$"
},
{
"author": "Lars Hernquist$^{3,4}$"
},
{
"author": "Neal Katz$^{5}$"
},
{
"author": "and Max Pettini$^{6}$"
}
] | We combine COBE-DMR measurements of cosmic microwave background (CMB) anisotropy with a recent measurement of the mass power spectrum at redshift $z=2.5$ from \lya\ forest data to derive constraints on cosmological parameters and test the inflationary cold dark matter (CDM) scenario of structure formation. By treating ... | [
{
"name": "ms.tex",
"string": "\\documentstyle[11pt,aaspp4]{article} \n\n\\newcommand{\\hmpc}{{h^{-1}{\\rm Mpc}\\;}}\n\\newcommand{\\kps}{{\\rm{km\\;s^{-1}\\;}}}\n\\newcommand{\\lya}{{Ly$\\alpha$}}\n\\newcommand{\\Onot}{{\\Omega_{m}}}\n\\newcommand{\\OLam}{{\\Omega_{\\Lambda}}}\n\\newcommand{\\Ob}{{\\Omega_... | [
{
"name": "astro-ph0001089.extracted_bib",
"string": "\\begin{thebibliography}{zaldariagga99}\n\n\\bibitem[Bahcall et al.\\ 1999]{bahcall99}\nBahcall, N. A., Ostriker, J. P., Perlmutter, S., \\& Steinhardt, P. J. 1999,\nScience, 284, 1481\n% cosmic triangle\n\n\\bibitem[Bardeen et al. 1986]{bardeen86}\nBard... |
astro-ph0001090 | Emission Lines in the Spectrum of the $^3$He Star 3 Cen A \footnote{Based on observations obtained with the Canada-France-Hawaii telescope, operated by the National Research Council of Canada, the Centre National de Scientifique of France, and the University of Hawaii.} | [
{
"author": "T.\\ A.\\ A.\\ Sigut"
},
{
"author": "J.\\ D.\\ Landstreet and S.\\ L.\\ S.\\ Shorlin"
}
] | Emission in the $4d\rightarrow 4f$ transitions of \ion{Mn}{2} (multiplet 13, $\lambda\lambda\,6122-6132\,$\AA), in the $4f\rightarrow 6g$ transitions of \ion{P}{2}, and in $\lambda\,6149.5$ of \ion{Hg}{2} has been detected in the spectrum of the helium weak star 3~Centauri~A (B5 III-IVp). Weaker emission from the same ... | [
{
"name": "submit_apjl.tex",
"string": "%\n% *************************************************************\n% Originally submitted to ApJ (Letters) 8 November 1999\n% Submitted in Revised form ApJ (Letters) 15 Dec 1999\n%\n% Questions? Problems? Contact Aaron Sigut at\n%\n% E-mail : asigut@inverse.astro.uwo... | [] |
astro-ph0001091 | X-ray observations of the high magnetic field radio pulsar PSR J1814$-$1744 | [
{
"author": "M. J. Pivovaroff"
},
{
"author": "V. M. Kaspi\\altaffilmark{1}"
}
] | PSR~J1814$-$1744 is a 4~s radio pulsar with surface dipole magnetic field strength $5.5 \times 10^{13}$~G, inferred assuming simple magnetic dipole braking. This pulsar's spin parameters are very similar to those of anomalous X-ray pulsars (AXPs), suggesting that this may be a transition object between the radio pulsar... | [
{
"name": "pkc00.tex",
"string": "%%\\documentstyle[12pt,aasms4,flushrt,psfig]{article}\n\\documentstyle[aas2pp4,flushrt]{article}\n\n\n%\\documentstyle[times,emulateapj,psfig]{article}\n%\\newcommand{\\PSbox}[3]{\\mbox{\\rule{0in}{#3}\\special{psfile=#1}\\hspace{#2}}}\n\n\\renewcommand{\\baselinestretch}{1... | [
{
"name": "astro-ph0001091.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[Arzoumanian {et al.} 1994]{antt94}\nArzoumanian, Z., Nice, D.~J., Taylor, J.~H., \\& Thorsett, S.~E. 1994,\n Astrophys. J., 422, 671\n\n\\bibitem[Becker \\& Tr\\\"{umper} 1997]{bt97}\nBecker, W. \\& Tr\\\"{umper}... |
astro-ph0001092 | Hubble Space Telescope imaging and ground-based spectroscopy of old nova shells -- I. FH Ser, V533 Her, BT Mon, DK Lac, V476 Cyg | [
{
"author": "C.D.\\ Gill$^1$ \\& T.J.\\ O'Brien$^2$"
},
{
"author": "Twelve Quays House"
},
{
"author": "Egerton Wharf"
},
{
"author": "Birkenhead"
},
{
"author": "L41 1LD"
},
{
"author": "2. Jodrell Bank Observatory"
},
{
"author": "Macclesfield"
},
{
"au... | In this paper we report on the first five out of eleven observations in our programme of Hubble Space Telescope (HST) imaging of old nova shells. We present new WFPC2 images of the shells around FH Ser and V533 Her taken in the F656N (H$\alpha$+[N~II]) filter. We also show long-slit spectra taken using the William Hers... | [
{
"name": "hst1.tex",
"string": "\\documentstyle{mn}\n\\begin{document}\n\\title\n[HST imaging and ground-based spectroscopy of nova shells -- I] \n{Hubble Space Telescope\nimaging and ground-based spectroscopy of old nova shells -- I. \nFH Ser, V533 Her, BT Mon, DK Lac, V476 Cyg}\n\\author[C.D.\\ Gill \\& ... | [
{
"name": "astro-ph0001092.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\n\\bibitem[\\protect\\citename{Bode }1989]{b1}\n Bode M. F., Evans A., 1989, Classical Novae, Wiley \\& Sons Ltd.,\n Chichester\n\n\\bibitem[\\protect\\citename{Borra}1970]{borra}\nBorra E.F., Andersen P.H., 1970, PASP, 82,... |
astro-ph0001093 | Chemo - Photometric evolution of star forming disk galaxy | [
{
"author": "Peter Berczik"
}
] | The chemical and photometric evolution of star forming disk galaxies is investigated. Numerical simulations of the complex gasdynamical flows are based on our own coding of the Chemo - Dynamical Smoothed Particle Hydrodynamical (CD - SPH) approach, which incorporates the effects of star formation. As a first applicatio... | [
{
"name": "berp.tex",
"string": "%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% \n\n\\documentclass[a4paper]{eslab}\n\\usepackage{graphics}\n\n%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%\n\n\\def\\apj#1{{ApJ} {#1}}\n\\def\\apjs#1{{ApJS} {#1}}\... | [
{
"name": "astro-ph0001093.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[\\protect\\astroncite{Berczik \\& Kravchuk}{1996}]{BerK96}\nBerczik P., Kravchuk S.G., 1996, \\apss{245} 27\n\n\\bibitem[\\protect\\astroncite{Berczik}{1999}]{Ber99}\nBerczik P., 1999, \\aa{348} 371, ({\\tt astro-p... |
astro-ph0001094 | Photoionization of Galactic Halo Gas by Old Supernova Remnants | [
{
"author": "Jonathan D. Slavin\\altaffilmark{1}"
}
] | We present new calculations on the contribution from cooling hot gas to the photoionization of warm ionized gas in the Galaxy. We show that hot gas in cooling supernova remnants (SNRs) is an important source of photoionization, particularly for gas in the halo. We find that in many regions at high latitude this source ... | [
{
"name": "SF_paper_preprint.tex",
"string": "\\documentclass[11pt,preprint]{aastex}\n%\\lefthead{}\n%\\righthead{}\n\\slugcomment{Submitted to the Astrophysical Journal}\n\\shorttitle{Photoionization of Galactic Halo Gas by SNRs}\n\\shortauthors{Slavin, McKee \\& Hollenbach}\n%\n\\begin{document}\n%\n\\new... | [
{
"name": "astro-ph0001094.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[Arabadjis \\& Bregman(1999)]{AB99} Arabadjis, J.\\ S.,\n\\& Bregman, J.\\ N.\\ 1999, \\apj, 510, 806\n\n\\bibitem[Bakes \\& Tielens(1998)]{BT98} Bakes, E.\\ L.\\ O.\\ \\& Tielens, A.\\ G.\\\nG.\\ M.\\ 1998, \\apj, ... |
astro-ph0001095 | Phase Lag and Coherence Function of X-ray emission from Black Hole Candidate XTE J1550-564 | [
{
"author": "Wei Cui\\altaffilmark{1}"
},
{
"author": "Shuang Nan Zhang\\altaffilmark{2}"
},
{
"author": "and Wan Chen\\altaffilmark{3,4}"
}
] | We report the results from measuring the phase lag and coherence function of X-ray emission from black hole candidate (BHC) XTE J1550-564. These X-ray temporal properties have been recognized to be increasingly important in providing important diagnostics of the dynamics of accretion flows around black holes. For XTE J... | [
{
"name": "cuipap.tex",
"string": "%\\documentstyle[aasms4]{article}\n\\documentstyle[11pt,aaspp4,epsfig]{article}\n\\slugcomment{To appear in Astrophysical Journal Letters}\n\n\\begin{document}\n\n\\title{Phase Lag and Coherence Function of X-ray emission from Black \nHole Candidate XTE J1550-564}\n\\autho... | [] |
astro-ph0001096 | Mapping the evolution of high redshift dusty galaxies with submillimeter observations of a radio-selected sample | [
{
"author": "A.\\"
},
{
"author": "J.\\ Barger"
},
{
"author": "$\\!$\\altaffilmark{1,2,3,4} L.\\"
},
{
"author": "L.\\ Cowie"
},
{
"author": "$\\!$\\altaffilmark{1,4} E.\\"
},
{
"author": "A.\\ Richards"
},
{
"author": "\\altaffilmark{2,4,5}"
}
] | Direct submillimeter imaging has recently revealed the 850\ $\mu$m background to be mostly composed of a population of distant ultraluminous infrared galaxies, but identifying the optical/near-infrared (NIR) counterparts to these sources has proved difficult due to the poor submillimeter spatial resolution. However, th... | [
{
"name": "ajb.tex",
"string": "%\\documentstyle[psfig,aasms4]{article}\n\\documentstyle[psfig,emulateapj]{article}\n\n\\lefthead{Barger et al.}\n\n\\begin{document}\n\\title{Mapping the evolution of high redshift dusty galaxies with\nsubmillimeter observations of a radio-selected sample\n}\n\\author{A.\\,J... | [] |
astro-ph0001097 | HST NICMOS Observation of Proto-Planetary Nebulae | [
{
"author": "Kate Y.L. Su"
},
{
"author": "Sun Kwok"
}
] | We report NICMOS wide-band and polarimetric observations of four proto-planetary nebulae. Molecular hydrogen emission is detected near the ends of the bipolar lobes of IRAS 17150-3224, which is evidence for the interaction of a fast, collimated outflow with the remnant of the asymptotic giant branch wind. | [
{
"name": "aspn-nic2.tex",
"string": "\\documentstyle[11pt,newpasp,twoside,epsf]{article}\n\\markboth{Su et al.}{NICMOS Observations of PPN}\n\\pagestyle{myheadings}\n\\nofiles\n\n% Some definitions I use in these instructions.\n\n\\def\\emphasize#1{{\\sl#1\\/}}\n\\def\\arg#1{{\\it#1\\/}}\n\\let\\prog=\\arg... | [] |
astro-ph0001098 | [
{
"author": "% %Begin Author names Omar Almaini %End Author names"
}
] | It is widely believed that most of the cosmic X-ray background (XRB) is produced by a vast, hitherto undetected population of obscured AGN. Deep X-ray surveys with Chandra and XMM will soon test this hypothesis. Similarly, recent sub-mm surveys with SCUBA have revealed an analogous population of exceptionally luminous,... | [
{
"name": "almaini.tex",
"string": "%\\documentstyle[psfig,epsf,conf-X,10pt]{article}\n%\n\\documentclass[10pt]{article}\n\\usepackage{psfig,epsf,conf-X}\n\n\\begin{document} \n\\small\n%\n\\heading{%\n%Begin Heading\n%\nThe X-ray/submillimetre Link\n% End Heading\n}\n\\par\\medskip\\noindent\n%\n\\author{%... | [
{
"name": "astro-ph0001098.extracted_bib",
"string": "\\bibitem{akiyama98} Akiyama M. et al, 1998, AN, 319, 63A\n\n\n\\bibitem{oa95}Almaini O., Boyle B.J., Griffiths R.E., Shanks T.,\nStewart G.C. \\& Georgantopoulos I., 1995, MNRAS 277, L31\n\n\n\\bibitem{oa96}Almaini O. et al., 1996, MNRAS, 282, 295\n\n... | |
astro-ph0001099 | Biased Estimates of $\Omega$ from Comparing Smoothed Predicted Velocity Fields to Unsmoothed Peculiar Velocity Measurements | [
{
"author": "Andreas A. Berlind"
},
{
"author": "Vijay K. Narayanan \\altaffilmark{1} and David H. Weinberg"
}
] | We show that a regression of unsmoothed peculiar velocity measurements against peculiar velocities predicted from a smoothed galaxy density field leads to a biased estimate of the cosmological density parameter $\Omega$, even when galaxies trace the underlying mass distribution and galaxy positions and velocities are k... | [
{
"name": "berlind.tex",
"string": "\\documentstyle[11pt,aasms4]{article}\n\n\\def\\baselinestretch{0.98}\n\n\\newcommand{\\vx}{{\\bf x}}\n\\newcommand{\\vxp}{{\\bf x^\\prime}}\n\\newcommand{\\vv}{{\\bf v}}\n\\newcommand{\\vk}{{\\bf k}}\n\\newcommand{\\divg}{{\\vec\\nabla}\\cdot}\n\\newcommand{\\vpred}{{\\b... | [
{
"name": "astro-ph0001099.extracted_bib",
"string": "\\begin{thebibliography}{blah99}\n\n\\bibitem[Berlind, Narayanan \\& Weinberg 1999; Berlind, Narayanan \\& Weinberg,\nin preparation]{berlind99}\nBerlind, A. A., Narayanan, V. K., \\& Weinberg, D. H. 1999, in ASP conference \nseries, Cosmic Flows, eds. S... |
astro-ph0001100 | Spectral Energy Distributions for Disk and Halo M--Dwarfs | [
{
"author": "S.K. Leggett"
}
] | We have obtained infrared (1---2.5$\mu$m) spectroscopy for 42 halo and disk dwarfs with spectral type M1 to M6.5. These data are compared to synthetic spectra generated by the latest model atmospheres of Allard \& Hauschildt. Photospheric parameters metallicity, effective temperature and radius are determined for the s... | [
{
"name": "prepr.tex",
"string": "%\\documentstyle[12pt,aasms4]{article}\n\\documentstyle[11pt,aaspp4]{article}\n%\\documentstyle[aas2pp4]{article}\n%\\documentstyle[12pt,amssym,aasms4]{article}\n \n%\\received{4 August 1988}\n%\\accepted{23 September 1988}\n%\\journalid{337}{15 January 1989}\n%\\articleid{... | [
{
"name": "astro-ph0001100.extracted_bib",
"string": "\\begin{thebibliography}{}\n\n\\bibitem[Allard et al. 1997]{all97} Allard, F., Hauschildt, P.H., Alexander, \nD.R., \\& Starrfield, S., 1997, \\araa, 35, 137 \n\\bibitem[Allard, Hauschildt \\& Schwenke 2000]{ahs99} Allard, F.,\nHauschildt, P.H. \\& Schw... |
astro-ph0001101 | CCD PHOTOMETRY OF THE GLOBULAR CLUSTER\\ $\omega$ CENTAURI.\\ I. METALLICITY OF RR LYRAE STARS FROM $Caby$ PHOTOMETRY\\ | [
{
"author": "Soo-Chang Rey\\altaffilmark{1}"
},
{
"author": "Young-Wook Lee"
},
{
"author": "and Jong-Myung Joo\\altaffilmark{1}"
}
] | We present new measurements of the metallicity of 131 RR Lyrae stars in the globular cluster $\omega$ Centauri, using the $hk$ index of the $Caby$ photometric system. The $hk$ method has distinct advantages over $\Delta$$S$ and other techniques in determining the metallicity of RR Lyrae stars, and has allowed us to obt... | [
{
"name": "Rey.tex",
"string": "% Rey.tex : Rey et al.\n\n%\\documentstyle[12pt,aasms4]{article}\n\\documentstyle[11pt,aaspp4]{article}\n\n%\\slugcomment{}\n\n\n\\lefthead{Soo-Chang Rey et al.}\n\\righthead{RR Lyrae stars in the $\\omega$ Centauri}\n\n\n\n\\begin{document}\n\\title{CCD PHOTOMETRY OF THE GLO... | [] |
astro-ph0001102 | RR Lyrae Variables in the Globular Cluster M5 | [
{
"author": "J. Kaluzny\\inst{1}"
},
{
"author": "~A. Olech\\inst{2}"
},
{
"author": "~I. Thompson\\inst{3}"
},
{
"author": "~W. Pych\\inst{2}"
},
{
"author": "~W. Krzeminski\\inst{1,3}"
},
{
"author": "~A. Schwarzenberg-Czerny\\inst{1,4}"
}
] | We present $V$-band CCD photometry of 65 RR Lyr variables from the globular cluster M5. We have estimated the basic physical parameters for 16 RRc stars and 26 RRab stars using a Fourier decomposition of the light curves of the variables. The mean values of mass, luminosity, effective temperature and relative helium ab... | [
{
"name": "m5h.tex",
"string": "\\documentstyle{l-aa}\n\\begin{document}\n\\thesaurus{08(08.22.3,08.06.3)}\n\\title{RR Lyrae Variables in the Globular Cluster M5}\n\\author{J. Kaluzny\\inst{1}, ~A. Olech\\inst{2}, ~I. Thompson\\inst{3}, \n~W. Pych\\inst{2},\n~W. Krzeminski\\inst{1,3} \\and ~A. Schwarzenberg... | [
{
"name": "astro-ph0001102.extracted_bib",
"string": "\\begin{thebibliography}{}\n \n\\bibitem[1975]{butler}\nButler, D., 1975, ApJ, 200, 68.\n\\bibitem[1999]{cap}\nCaputo, F., Castellani, V., Marconi, M., Ripepi, V., 1999, accepted for\npublication in MNRAS (astro-ph/9902279)\n\\bibitem[1992]{car}\nCarney,... |