Neutron Star Model Atmospheres

Details Neutron Star Model Atmospheres Neutron Star Model Atmospheres

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1171..343s&link_type=abstract

RECENT DIRECTIONS IN ASTROPHYSICAL QUANTITATIVE SPECTROSCOPY AND RADIATION HYDRODYNAMICS: Proceedings of the International Confe

Astronomy and Astrophysics

Astrophysics

Neutron Stars, Stellar Atmospheres, Accretion Disks, Neutron Stars, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation, Infall, Accretion, And Accretion Disks

Scientific paper

Determination of neutron star (NS) parameters is an important astrophysical problem. The stellar radius depends on the mass and the equation of state (EOS) in the NS core, which is not well known. Therefore, with masses and radii inferred from observations we are able to select between various theories for the EOS. Theoretical models of NS spectra are needed for this purpose.

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