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pubmed-article:12815425pubmed:issue6942lld:pubmed
pubmed-article:12815425pubmed:dateCreated2003-6-19lld:pubmed
pubmed-article:12815425pubmed:abstractTextOver the past five years evidence has mounted that long-duration (>2 s) gamma-ray bursts (GRBs)-the most luminous of all astronomical explosions-signal the collapse of massive stars in our Universe. This evidence was originally based on the probable association of one unusual GRB with a supernova, but now includes the association of GRBs with regions of massive star formation in distant galaxies, the appearance of supernova-like 'bumps' in the optical afterglow light curves of several bursts and lines of freshly synthesized elements in the spectra of a few X-ray afterglows. These observations support, but do not yet conclusively demonstrate, the idea that long-duration GRBs are associated with the deaths of massive stars, presumably arising from core collapse. Here we report evidence that a very energetic supernova (a hypernova) was temporally and spatially coincident with a GRB at redshift z = 0.1685. The timing of the supernova indicates that it exploded within a few days of the GRB, strongly suggesting that core-collapse events can give rise to GRBs, thereby favouring the 'collapsar' model.lld:pubmed
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pubmed-article:12815425pubmed:authorpubmed-author:JakobssonTell...lld:pubmed
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pubmed-article:12815425pubmed:day19lld:pubmed
pubmed-article:12815425pubmed:volume423lld:pubmed
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pubmed-article:12815425pubmed:pagination847-50lld:pubmed
pubmed-article:12815425pubmed:dateRevised2003-11-4lld:pubmed
pubmed-article:12815425pubmed:year2003lld:pubmed
pubmed-article:12815425pubmed:articleTitleA very energetic supernova associated with the gamma-ray burst of 29 March 2003.lld:pubmed
pubmed-article:12815425pubmed:affiliationAstronomical Observatory, NBIfAFG, University of Copenhagen, Juliane Maries Vej, DK-2100 Copenhagen Ø, Denmark. jens@astro.ku.dklld:pubmed
pubmed-article:12815425pubmed:publicationTypeJournal Articlelld:pubmed
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