J/AcA/41/73ivo://CDS.VizieR/J/AcA/41/73doi:10.26093/cds/vizier.120410073CDSMadej J.2025-09-25T20:14:15Z2014-11-19T08:04:54ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frastronomical-modelsstellar-atmospheresx-ray-binary-starsX-ray burst sources represent a class of accreting neutron stars in close binary systems which do not exhibit any traces of the magnetic field. We present the first detailed tables which show the structure of plane--parallel hydrogen-helium atmospheres of bursting neutron stars. Hydrogen-helium models were computed with precise angle-dependent radiative transfer under constrains of radiative and hydrostatic equilibrium. Compton scattering opacity included both the Klein-Nishina corrections and the effects of relativistic Maxwellian thermal motion of scattering electrons. Compton redistribution function allows for large energy exchange between X-ray photons and scattering electrons.1991AcA....41...73Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AcA/41/73CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AcA/41/73https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AcA/41/73http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AcA/41/73https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AcA/41/73https://vizier.iucaa.in/viz-bin/votable?-source=J/AcA/41/73http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AcA/41/73GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/AcA/41/73/listModel parametersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeffEffective temperature (8.00E+06, 1.257E+07, 2.00E+07, 3.00E+07)Kphys.temperature.effectivedoubleloggLogarithm of surface gravity (12.5 to 15.0)log(cm.s**-2)phys.gravityfloatnr[1/20] Model numbermeta.id;meta.mainintJ/AcA/41/73/table1*Run of physical variablesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnr[1/20] Model numbermeta.id;meta.maininttau-stdStandard optical depthstat.error;stat.stdevdoubleTempTemperature (1)Kphys.temperaturedoublePGGas pressure (1)dyn.cm**-2phys.pressuredoubleAcc-radRadiative acceleration (1)cm.s**-2physdoubleneElectron concentration (1)cm**-3phys.densitydoublerhoGas density (1)g.cm**-3phys.densitydoubletau-RossRosseland optical depthphys.absorption.opticalDepthdoubleHeightgeometrical height (1)cmpos.cartesian.zdouble