Gamma-Ray Bursts: Astronomical Constraints

dc.creatorPostnov, K. A.
dc.date2000-10-02
dc.date2000-10-09
dc.date.accessioned2026-07-07T01:55:45Z
dc.date.available2026-07-07T01:55:45Z
dc.descriptionAfter presenting a short history of gamma-ray burst (GRB) studies, we discuss the current constraints on GRB models which follows from astronomical observations. We concentrate on the energetics of the GRBs with known redshifts and the association of the well-localized GRBs with star forming regions in remote galaxies. We also discuss implications of the observed GRB rate. Arguments are given favoring possible connection of GRBs with core collapse of massive Wolf-Rayet stars. The possibility of GRB to be a transient phenomenon in the early history of galactic star formation related to evolution of very massive metal-free stars is briefly outlined.
dc.description14 pages, 2 Postscript figures, uses epsf.sty. To appear in Proc. Bogolyubov Theoretical Physics Laboratory of JINR (Dubna) Workshop "Hot topics in astrophysics", August 2000 Table 1 completed, Fig. 1 changed, some references added
dc.identifierhttps://arxiv.org/abs/astro-ph/0010031
dc.identifierhttp://arxiv.org/abs/astro-ph/0010031
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1767
dc.subjectAstrophysics
dc.titleGamma-Ray Bursts: Astronomical Constraints
dc.typetext

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