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Nucleosynthesis in helium-enriched asymptotic giant branch models: Implications for heavy element enrichment in ω centauri

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dc.contributor.authorKarakas, Amanda
dc.contributor.authorMarino, Anna
dc.contributor.authorNataf, David
dc.date.accessioned2015-12-10T23:20:17Z
dc.date.issued2014
dc.date.updated2015-12-10T10:22:02Z
dc.description.abstractWe investigate the effect of helium enrichment on the evolution and nucleosynthesis of low-mass asymptotic giant branch (AGB) stars of 1.7 Mand 2.36 Mwith a metallicity of Z = 0.0006 ([Fe/H] ≈-1.4). We calculate evolutionary sequences with the primordia
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/66256
dc.publisherIOP Publishing
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstrophysical Journal, The
dc.titleNucleosynthesis in helium-enriched asymptotic giant branch models: Implications for heavy element enrichment in ω centauri
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage12
local.bibliographicCitation.startpage32/1
local.contributor.affiliationKarakas, Amanda, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMarino, Anna, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationNataf, David, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidKarakas, Amanda, u4382192
local.contributor.authoruidMarino, Anna, u5239722
local.contributor.authoruidNataf, David, u5239355
local.description.notesImported from ARIES
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.ariespublicationU3488905xPUB1252
local.identifier.citationvolume784
local.identifier.doi10.1088/0004-637X/784/1/32
local.identifier.scopusID2-s2.0-84896743712
local.identifier.thomsonID000335457000032
local.type.statusPublished Version

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