A new model of gamma-ray burst

Details A new model of gamma-ray burst A new model of gamma-ray burst

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994cha%26a..18..266w&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 18, Issue 3, p. 266-271.

Astronomy and Astrophysics

Astrophysics

Neutron Stars, Γ Burst, Radiative Transfer

Scientific paper

We propose a new model of γ burst, based on the assumption that it originates in old neutron stars. We assume that the surface magnetic field of an old neutron star consists of two parts, one is a weak background dipole field, the other is strong, local, tube-like fields. This model can explain both the absorption features and the high-energy tail in the spectrum. Our model gives a good fit to the observed spectrum of GB 880205

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