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Are the precursors of type IA supernovae double degenerate mergers?

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dc.contributor.authorFerrario, Liliaen
dc.date.accessioned2025-06-24T03:35:43Z
dc.date.available2025-06-24T03:35:43Z
dc.date.issued2004en
dc.description.abstractI argue that the observational evidence for white dwarf-white dwarf mergers supports the view that they give rise to ultra-massive white dwarfs or neutron stars through accretion induced collapse. The implications for the progenitors of Type Ia SNe are discussed.en
dc.description.statusPeer-revieweden
dc.format.extent2en
dc.identifier.issn1405-2059en
dc.identifier.otherORCID:/0000-0002-0485-0518/work/162369275en
dc.identifier.scopus11844306865en
dc.identifier.urihttp://www.scopus.com/inward/record.url?scp=11844306865&partnerID=8YFLogxKen
dc.identifier.urihttps://hdl.handle.net/1885/733764654
dc.language.isoenen
dc.relation.ispartofseriesIAU Colloquium 194 - Compact Binaries in the Galaxy and Beyonden
dc.sourceRevista Mexicana de Astronomia y Astrofisica: Serie de Conferenciasen
dc.subjectStars: Neutronen
dc.subjectStars: Supernovaeen
dc.subjectWhite dwarfsen
dc.titleAre the precursors of type IA supernovae double degenerate mergers?en
dc.typeConference paperen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage112en
local.bibliographicCitation.startpage111en
local.contributor.affiliationFerrario, Lilia; Mathematics Programs, Mathematical Sciences Institute, ANU College of Systems and Society, The Australian National Universityen
local.identifier.ariespublicationMigratedxPub16166en
local.identifier.citationvolume20en
local.identifier.doi10.1017/s025292110015211xen
local.identifier.pure5ad406bc-ec8d-4125-8e09-7077bfa59096en
local.identifier.urlhttps://www.scopus.com/pages/publications/11844306865en
local.type.statusPublisheden

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