Model atmospheres for neutron stars

Details Model atmospheres for neutron stars Model atmospheres for neutron stars

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.255..129m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 255, March 1, 1992, p. 129-145. Research supported by U

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51

Neutron Stars, Stellar Atmospheres, Stellar Models, Supernova 1987A, Computational Astrophysics, Rosat Mission, Spaceborne Astronomy, Stellar Magnetic Fields, Stellar Radiation

Scientific paper

Many neutron stars are expected to have extremely high magnetic fields. This paper uses atomic data in high magnetic fields computed using a multiconfigurational Hartree-Fock code, and the data were presented in Miller and Neuhauser. The effects of ionization and polarization in strong magnetic fields are discussed, and the prospects for observation by satellites are investigated.

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