Radiative opacities and photosphere models for soft gamma repeaters

Details Radiative opacities and photosphere models for soft gamma repeaters Radiative opacities and photosphere models for soft gamma repeaters

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..384..907b&link_type=abstract

Gamma-ray bursts: 3rd Huntsville symposium. AIP Conference Proceedings, Volume 384, pp. 907-912 (1996).

Physics

15

Radiative Transfer, Scattering, Gamma-Ray Sources, Gamma-Ray Bursts, Neutron Stars, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation

Scientific paper

We consider the radiative processes for conditions expected in photospheres of neutron stars (NSs) with magnetic fields B~1014-1016 G. The radiative opacities are employed to construct model photospheres and to calculate the spectral flux and specific intensity emitted by these objects which are thought to be associated with Soft Gamma Repeaters (SGRs).

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