What made GRBs 060505 and 060614?

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dc.creatorJakobsson, P.
dc.creatorFynbo, J. P. U.
dc.date2007-04-11
dc.date.accessioned2026-07-07T07:56:09Z
dc.date.available2026-07-07T07:56:09Z
dc.descriptionRecent observations of two nearby SN-less long-duration gamma-ray bursts (GRBs), which share no obvious characteristics in their prompt emission, suggest a new phenomenological type of massive stellar death. Here we briefly review the observational properties of these bursts and their proposed hosts, and discuss whether a new GRB classification scheme is needed.
dc.description4 pages, 1 figure. Proceedings of the Amsterdam RTN (GRBs: an enigma and a tool) meeting, March 19-23, 2007. To appear in New Astronomy Reviews
dc.identifierhttps://arxiv.org/abs/0704.1421
dc.identifierhttp://arxiv.org/abs/0704.1421
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/127206
dc.subjectAstrophysics
dc.titleWhat made GRBs 060505 and 060614?
dc.typetext

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