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A common envelope binary star origin of long gamma-ray bursts

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dc.contributor.authorTout, Christopher A
dc.contributor.authorWickramasinghe, Dayal
dc.contributor.authorLau, Herbert H-B
dc.contributor.authorPringle, James
dc.contributor.authorFerrario, Lilia
dc.date.accessioned2015-12-10T23:19:21Z
dc.date.issued2011
dc.date.updated2016-02-24T08:10:06Z
dc.description.abstractThe stellar origin of γ-ray bursts can be explained by the rapid release of energy in a highly collimated, extremely relativistic jet. This in turn appears to require a rapidly spinning highly magnetized stellar core that collapses into a magnetic neutro
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/65888
dc.publisherBlackwell Publishing Ltd
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Binaries: close; Gamma-ray burst: general; Stars: neutron; White dwarfs
dc.titleA common envelope binary star origin of long gamma-ray bursts
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue4
local.bibliographicCitation.lastpage2462
local.bibliographicCitation.startpage2458
local.contributor.affiliationTout, Christopher A, University of Cambridge
local.contributor.affiliationWickramasinghe, Dayal, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLau, Herbert H-B, Monash University
local.contributor.affiliationPringle, James, Cambridge Institute of Astronomy
local.contributor.affiliationFerrario, Lilia, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidWickramasinghe, Dayal, u7600909
local.contributor.authoruidFerrario, Lilia, u8513121
local.description.notesImported from ARIES
local.identifier.absfor020106 - High Energy Astrophysics; Cosmic Rays
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationf2965xPUB1179
local.identifier.citationvolume410
local.identifier.doi10.1111/j.1365-2966.2010.17622.x
local.identifier.scopusID2-s2.0-78751631757
local.identifier.thomsonID000286211000030
local.type.statusPublished Version

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