X-ray spectra from convective photospheres of neutron stars

Simple item page
dc.creatorZavlin, V. E.
dc.creatorPavlov, G. G.
dc.creatorShibanov, Yu. A.
dc.creatorRogers, F. J.
dc.creatorIglesias, C. A.
dc.date1995-10-23
dc.date1995-11-09
dc.date.accessioned2026-07-07T08:58:22Z
dc.date.available2026-07-07T08:58:22Z
dc.descriptionWe present first results of modeling convective photospheres of neutron stars. We show that in photospheres composed of the light elements convection arises only at relatively low effective temperatures (< 3-5*10^4 K), whereas in the case of iron compositon it arises at < 3*10^ K. Convection changes the depth dependence of the photosphere temperature and the shapes of the emergent spectra. Thus, it should be taken into account for the proper interpretation of EUV/soft-X-ray observations of the thermal radiation from neutron stars.
dc.description2 pages, from Wuerzburg X-ray Conference (Sep. 25-29, 1995); final version; ask for psfile to: zavlin@rosat.mpe-garching.mpg.de
dc.identifierhttps://arxiv.org/abs/astro-ph/9510116
dc.identifierhttp://arxiv.org/abs/astro-ph/9510116
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147298
dc.subjectAstrophysics
dc.titleX-ray spectra from convective photospheres of neutron stars
dc.typetext

Files

Collections

arXiv