Evolution and nucleosynthesis of asymptotic giant branch stellar models of low metallicity

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dc.contributor.authorFishlock, Cherie
dc.contributor.authorKarakas, Amanda
dc.contributor.authorLugaro, Maria
dc.contributor.authorYong, David
dc.date.accessioned2015-12-13T22:34:36Z
dc.date.issued2014
dc.date.updated2015-12-11T09:22:35Z
dc.description.abstractWe present stellar evolutionary tracks and nucleosynthetic predictions for a grid of stellar models of low- and intermediate-mass asymptotic giant branch (AGB) stars at Z = 0.001 ([Fe/H] =-1.2). The models cover an initial mass range from 1 M⊙ to 7 M⊙
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/76202
dc.publisherIOP Publishing
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstrophysical Journal, The
dc.titleEvolution and nucleosynthesis of asymptotic giant branch stellar models of low metallicity
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue44
local.bibliographicCitation.startpage25
local.contributor.affiliationFishlock, Cherie, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationKarakas, Amanda, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLugaro, Maria, Monash University
local.contributor.affiliationYong, David, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidFishlock, Cherie, u4927594
local.contributor.authoruidKarakas, Amanda, u4382192
local.contributor.authoruidYong, David, u3207952
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationU3488905xPUB5062
local.identifier.citationvolume797
local.identifier.doi10.1088/0004-637X/797/1/44
local.identifier.scopusID2-s2.0-84914703021
local.identifier.thomsonID000345915000044
local.type.statusPublished Version

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