GRB 120422A/SN 2012bz: Bridging the gap between low- and high-luminosity gamma-ray bursts

dc.contributor.author	Schulze, S., et al.
dc.contributor.author	Pandey, S. B.
dc.date.accessioned	2019-07-01T09:33:49Z
dc.date.available	2019-07-01T09:33:49Z
dc.date.issued	2014-06
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/1227
dc.description.abstract	At low redshift, a handful of gamma-ray bursts (GRBs) have been discovered with luminosities that are substantially lower (Liso ≲ 1048.5 erg s-1) than the average of more distant ones (Liso ≳ 1049.5 erg s-1). It has been suggested that the properties of several low-luminosity (low-L) GRBs are due to shock break-out, as opposed to the emission from ultrarelativistic jets. This has led to much debate about how the populations are connected.	en_US
dc.language.iso	en_US	en_US
dc.publisher	EDP Sciences	en_US
dc.relation.ispartofseries	aa566-A102;
dc.subject	gamma-ray burst	en_US
dc.subject	Supernovae	en_US
dc.subject	Galaxies	en_US
dc.title	GRB 120422A/SN 2012bz: Bridging the gap between low- and high-luminosity gamma-ray bursts	en_US
dc.type	Article	en_US