Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-08-19
Astronomy and Astrophysics
Astrophysics
Apj in press: 25 pages, 16 figures
Scientific paper
10.1086/307471
We present a phenomenological model to explain the light curves of gamma-ray bursts. In the model a black hole is orbited by a precessing accretion disc which is fed by a neutron star. Gamma-rays are produced in a highly collimated beam via the Blandford-Znajek mechanism. The gamma-ray beam sweeps through space due to the precession of the slaved accretion disc. The light curve expected from such a precessing luminosity cone can explain the complex temporal behavior of observed bright gamma-ray bursts.
Lee Chang-Hwan
Lee Hyun Kyu
Portegies Zwart Simon
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