Explaining the light curves of Gamma-ray Bursts with precessing jets

Astronomy and Astrophysics – Astrophysics

Scientific paper

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2 pages, to be publishes in the Rome Conference: Gamma Ray Bursts in the Afterglow Era

Scientific paper

10.1051/aas:1999326

A phenomenological model is presented to explain the light curves of
gamma-ray bursts. Gamma-rays are produced in a narrow beam which sweeps through
space due to the precession of a slaved accretion disc. The light curve
expected from such a precessing luminosity cone can explain the complex
temporal behavior of bright gamma-ray bursts.

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