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Title:
An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova
Authors:
Della Valle, M.; Chincarini, G.; Panagia, N.; Tagliaferri, G.; Malesani, D.; Testa, V.; Fugazza, D.; Campana, S.; Covino, S.; Mangano, V.; Antonelli, L. A.; D'Avanzo, P.; Hurley, K.; Mirabel, I. F.; Pellizza, L. J.; Piranomonte, S.; Stella, L.
Publication:
Nature, Volume 444, Issue 7122, pp. 1050-1052 (2006). (Nature Homepage)
Publication Date:
12/2006
Origin:
NATURE
Abstract Copyright:
(c) 2006: Nature
DOI:
10.1038/nature05374
Bibliographic Code:
2006Natur.444.1050D

Abstract

Gamma-ray bursts (GRBs) are short, intense flashes of soft γ-rays coming from the distant Universe. Long-duration GRBs (those lasting more than ~2s) are believed to originate from the deaths of massive stars, mainly on the basis of a handful of solid associations between GRBs and supernovae. GRB 060614, one of the closest GRBs discovered, consisted of a 5-s hard spike followed by softer, brighter emission that lasted for ~100s (refs 8, 9). Here we report deep optical observations of GRB 060614 showing no emerging supernova with absolute visual magnitude brighter than MV=-13.7. Any supernova associated with GRB 060614 was therefore at least 100 times fainter, at optical wavelengths, than the other supernovae associated with GRBs. This demonstrates that some long-lasting GRBs can either be associated with a very faint supernova or produced by different phenomena.
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