Cyclotron lines in gamma-ray burst spectra - Absorption in a radiation-driven wind

Details Cyclotron lines in gamma-ray burst spectra - Absorption in a radiation-driven wind Cyclotron lines in gamma-ray burst spectra - Absorption in a radiation-driven wind

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvl..66.1395m&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 66, March 18, 1991, p. 1395-1397. DOE-supported research.

Astronomy and Astrophysics

Astronomy

19

Astronomical Spectroscopy, Cyclotron Radiation, Gamma Ray Bursts, Line Spectra, Neutron Stars, Cosmic Plasma, Cosmic Rays, Photons, Stellar Magnetic Fields

Scientific paper

Previous models of cyclotron-line features in the spectra of cosmic
gamma-ray bursts have assumed that the lines form in a thin static
atmosphere. It is shown that the observed absorption lines may in fact
form in a radiation-driven plasma wind expelled at relativistic
velocities from the surface of a neutron star.

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