Thermal Radiation From Isolated Neutron Stars

Details Thermal Radiation From Isolated Neutron Stars Thermal Radiation From Isolated Neutron Stars

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..801..259l&link_type=abstract

ASTROPHYSICAL SOURCES OF HIGH ENERGY PARTICLES AND RADIATION. AIP Conference Proceedings, Volume 801, pp. 259-264 (2005).

Astronomy and Astrophysics

Astrophysics

Neutron Stars, Stellar Magnetism, Stellar Atmospheres, Neutron Stars, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation

Scientific paper

The last few years have seen significant observational progress in the study of surface radiation from magnetic neutron stars, including radio pulsars, radio-quiet neutron stars and magnetars. Modeling such radiation requires a detailed understanding of the property of matter in strong magnetic fields and radiative processes in highly magnetized, birefringent plasmas. In this paper we review the current observations and discuss theoretical issues/challenges related to modeling neutron star atmospheres/surfaces.

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