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Are the precursors of type IA supernovae double degenerate mergers?

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dc.contributor.authorFerrario, Lilia
dc.coverage.spatialLa oaz
dc.date.accessioned2015-12-13T23:09:33Z
dc.date.available2015-12-13T23:09:33Z
dc.date.createdNovember 17 2003
dc.date.issued2004
dc.date.updated2015-12-12T08:19:40Z
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.
dc.identifier.isbn9703211585
dc.identifier.urihttp://hdl.handle.net/1885/87046
dc.publisherInstituto de Astronomia
dc.relation.ispartofseriesInternational Astronomical Union Symposium 194
dc.sourceRevista Mexicana de Astronomia y astrofisica
dc.source.urihttp://www.astroscu.unam.mx/~rmaa/rmaa.html
dc.subjectKeywords: Stars: Neutron; Stars: Supernovae; White dwarfs
dc.titleAre the precursors of type IA supernovae double degenerate mergers?
dc.typeConference paper
local.bibliographicCitation.lastpage112
local.bibliographicCitation.startpage111
local.contributor.affiliationFerrario, Lilia, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidFerrario, Lilia, u8513121
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub16166
local.identifier.scopusID2-s2.0-11844306865
local.type.statusPublished Version

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