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

1999-03-05

arxiv.org/abs/astro-ph/9903090v1

Astronomy and Astrophysics

Astrophysics

Talk at the Workshop "Gamma-Ray Bursts in the Afterglow Era", Rome, November 3-6. To appear in A&A Suppl

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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