Three-dimensional modelling of proton ingestion episodes in low-mass stars

dc.contributor.authorHeap, Stuart
dc.contributor.authorStancliffe, Richard
dc.contributor.authorLattanzio, John
dc.contributor.authorDearborn, David
dc.coverage.spatialCairns Australia
dc.date.accessioned2015-12-13T22:57:37Z
dc.date.createdAugust 5-12 2012
dc.date.issued2013
dc.date.updated2015-12-12T07:17:33Z
dc.description.abstractWe have modelled a dual shell flash (DSF) in a low-metallicity 1.5M ȯ AGB star using the 3-dimensional hydrodynamic program "Djehuty", observing how the evolution of these events compares to 1-dimensional models, which are hypothesised to be inaccurate d
dc.identifier.urihttp://hdl.handle.net/1885/83043
dc.publisherConference Organising Committee
dc.relation.ispartofseries12th International Symposium on Nuclei in the Cosmos, NIC 2012
dc.sourceProceedings of Science
dc.titleThree-dimensional modelling of proton ingestion episodes in low-mass stars
dc.typeConference paper
local.contributor.affiliationHeap, Stuart, Monash University
local.contributor.affiliationStancliffe, Richard , College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLattanzio, John, Monash University
local.contributor.affiliationDearborn, David, Lawrence Livermore National Laboratory
local.contributor.authoruidStancliffe, Richard , u5083819
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB11248
local.identifier.scopusID2-s2.0-84887495194
local.type.statusPublished Version

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