Origin of GRB afterglows in the model of galactic neutron stars

Details Origin of GRB afterglows in the model of galactic neutron stars Origin of GRB afterglows in the model of galactic neutron stars

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26as..138..551b&link_type=abstract

Astronomy and Astrophysics Supplement, v.138, p.551-552

Astronomy and Astrophysics

Astrophysics

1

Gamma-Ray: Bursts

Scientific paper

The launch of the Beppo-Sax satellite gave a unique opportunity to investigate gamma ray bursts (GRB) in different spectral regions. The large diversity of the afterglow behavior creates additional problems for the cosmological model with a fireball. Formation of the afterglow giving the observed diversity of properties is suggested in the Galactic neutron star model of GRBs. It is based on the transient accretion disc formation around the neutron star with a low-mass brown companion irradiated by the neutron star.

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