Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...344l...1a&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 344, Sept. 1, 1989, p. L1-L4. Research supported by the National
Astronomy and Astrophysics
Astronomy
44
Cyclotron Radiation, Gamma Ray Astronomy, Gamma Ray Bursts, Line Spectra, Magnetic Resonance, Quantum Electrodynamics, Radiative Transfer, Wave Scattering
Scientific paper
A transmission model of gamma-ray burst sources is studied using the relativistic QED magnetic-resonant opacities including multiple photon scattering, incorporated into a discrete-ordinate radiative-transport scheme. The physics of the cyclotron line-producing region is discussed in general, and the expected line profiles, relative harmonic strengths, and polarizations are indicated under various conditions. The calculated spectra for these models show good agreement with the spectra reported from Ginga for GB 880205 and GB 870303.
Alexander S. G.
Meszaros Peter
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