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Accretion induced collapse of white dwarfs in binary systems and their observational properties

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dc.contributor.authorWickramasinghe, Dayal
dc.contributor.authorHurley, Jarrod
dc.contributor.authorFerrario, Lilia
dc.contributor.authorTout, Christopher A
dc.contributor.authorKiel, Paul D
dc.date.accessioned2015-12-08T22:38:07Z
dc.date.issued2009
dc.date.updated2015-12-08T10:06:07Z
dc.description.abstractNeutron stars can form through core collapse (CC) following a supernova explosion of a massive star, or from a white dwarf that first forms in a binary system and then collapses into a neutron star via accretion induced collapse (AIC). So far, there have
dc.identifier.issn1742-6596
dc.identifier.urihttp://hdl.handle.net/1885/35814
dc.publisherInstitute of Physics Publishing
dc.sourceJournal of Physics: Conference Series
dc.titleAccretion induced collapse of white dwarfs in binary systems and their observational properties
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage4
local.bibliographicCitation.startpage1
local.contributor.affiliationWickramasinghe, Dayal, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationHurley, Jarrod, Swinburne University of Technology
local.contributor.affiliationFerrario, Lilia, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationTout, Christopher A, University of Cambridge
local.contributor.affiliationKiel, Paul D, Swinburne University of Technology
local.contributor.authoruidWickramasinghe, Dayal, u7600909
local.contributor.authoruidFerrario, Lilia, u8513121
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020199 - Astronomical and Space Sciences not elsewhere classified
local.identifier.ariespublicationu9209279xPUB128
local.identifier.citationvolume172
local.identifier.doi10.1088/1742-6596/172/1/012037
local.identifier.scopusID2-s2.0-68349137647
local.identifier.thomsonID000273522500037
local.type.statusPublished Version

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