V. I. Dokuchaev, Yu. N. Eroshenko
Published 2011-02-20Version 1
The probability of observing "supernova - gamma-ray burst" (GRB) pair events and recurrent GRBs from one galaxy in a time interval of several years has been estimated. Supernova explosions in binary systems accompanied by the formation of a short-lived pair of compact objects can be the sources of such events. If a short GRB is generated during the collision of a pair, then approximately each of ~300 short GRBs with redshift z must have an optical precursor - a supernova in the observer's time interval <2(1+z)yr. If the supernova explosion has the pattern of a hypernova, then a successive observation of long and short GRBs is possible. The scenario for the generation of multiple GRBs in collapsing galactic nuclei is also discussed.
Comments: 12 pages, 1 figure; this paper has the e-precursor arXiv:1101.3298 [astro-ph.HE]
Journal: Astronomy Letters 37, 83 (2011)
Radio Constraints on Long-Lived Magnetar Remnants in Short Gamma-Ray Bursts
The formation rate of short gamma-ray bursts and gravitational waves
The Jet Opening Angle and Event Rate Distributions of Short Gamma-ray Bursts from Late-time X-ray Afterglows
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