Sub-Chandrasekhar models for Type Ia supernovae and astrophysical transients

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dc.contributor.authorFink, M
dc.contributor.authorRopke, F. K.
dc.contributor.authorSim, Stuart A
dc.contributor.authorKromer, M
dc.contributor.authorSeitenzahl, I. R.
dc.contributor.authorRuiter, A. J.
dc.contributor.authorHillebrandt, Wolfgang
dc.coverage.spatialCairns Australia
dc.date.accessioned2015-12-13T22:57:31Z
dc.date.createdAugust 5-12 2012
dc.date.issued2013
dc.date.updated2015-12-12T07:16:59Z
dc.description.abstractSub-Chandrasekhar models aim to explain Type Ia supernovae from the explosion of white dwarf stars with masses below the Chandrasekhar limit. An advantage of this scenario is the wide range of possible progenitor masses, which may lead to a wide range of
dc.identifier.urihttp://hdl.handle.net/1885/83013
dc.publisherConference Organising Committee
dc.relation.ispartofseries12th International Symposium on Nuclei in the Cosmos, NIC 2012
dc.sourceProceedings of Science
dc.titleSub-Chandrasekhar models for Type Ia supernovae and astrophysical transients
dc.typeConference paper
local.contributor.affiliationFink, M, Max Planck Institut für Astrophysik
local.contributor.affiliationRopke, F. K., Max Planck Institut fur Astrophysik
local.contributor.affiliationSim, Stuart A, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationKromer, M, Max Planck Institut für Astrophysik
local.contributor.affiliationSeitenzahl, I. R., Max Planck Institut für Astrophysik
local.contributor.affiliationRuiter, A. J., Max Planck Institut für Astrophysik
local.contributor.affiliationHillebrandt, Wolfgang, Max Planck Institute for Astrophysics
local.contributor.authoruidSim, Stuart A, u4967042
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB11221
local.identifier.scopusID2-s2.0-84887469719
local.type.statusPublished Version

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