2D simulations of the double-detonation model for thermonuclear transients from low-mass carbon-oxygen white dwarfs

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dc.contributor.authorSim, Stuart A
dc.contributor.authorFink, M
dc.contributor.authorKromer, M
dc.contributor.authorRopke, F. K.
dc.contributor.authorRuiter, A. J.
dc.contributor.authorHillebrandt, Wolfgang
dc.date.accessioned2015-12-10T23:25:19Z
dc.date.issued2012
dc.date.updated2016-02-24T08:47:11Z
dc.description.abstractThermonuclear explosions may arise in binary star systems in which a carbon-oxygen (CO) white dwarf (WD) accretes helium-rich material from a companion star. If the accretion rate allows a sufficiently large mass of helium to accumulate prior to ignition
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/67577
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Binaries: close; Hydrodynamics; Methods: numerical; Radiative transfer; Supernovae: general; White dwarfs
dc.title2D simulations of the double-detonation model for thermonuclear transients from low-mass carbon-oxygen white dwarfs
dc.typeJournal article
local.bibliographicCitation.issue4
local.bibliographicCitation.lastpage3016
local.bibliographicCitation.startpage3003
local.contributor.affiliationSim, Stuart A, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationFink, M, Max Planck Institut für Astrophysik
local.contributor.affiliationKromer, M, Max Planck Institut für Astrophysik
local.contributor.affiliationRopke, F. K., Max Planck Institut fur Astrophysik
local.contributor.affiliationRuiter, A. J., Max Planck Institut für Astrophysik
local.contributor.affiliationHillebrandt, Wolfgang, Max Planck Institute for Astrophysics
local.contributor.authoremailu4967042@anu.edu.au
local.contributor.authoruidSim, Stuart A, u4967042
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationf5625xPUB1480
local.identifier.citationvolume420
local.identifier.doi10.1111/j.1365-2966.2011.20162.x
local.identifier.scopusID2-s2.0-84857651174
local.identifier.thomsonID000300935100021
local.identifier.uidSubmittedByf5625
local.type.statusPublished Version

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