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Carbon-enhanced metal-poor stars and the s/r process

dc.contributor.authorLugaro, Maria
dc.contributor.authorKarakas, Amanda
dc.contributor.authorStancliffe, Richard
dc.contributor.authorRijs, Carlos
dc.coverage.spatialWako, Japan
dc.date.accessioned2015-12-13T22:18:17Z
dc.date.createdNovember 14-17 2011
dc.date.issued2012
dc.date.updated2016-02-24T09:02:23Z
dc.description.abstractWe have performed calculations for the slow neutron capture process (the s process) in stellar models of mass from 0.9 M⊙ to 6 M ⊙ at a metallicity of [Fe/H]=-2.3. The models were computed with two different stellar evolution codes and our results com
dc.identifier.isbn9780735410961
dc.identifier.urihttp://hdl.handle.net/1885/71574
dc.publisherAmerican Institute of Physics
dc.relation.ispartofseriesInternational Symposium on Origin of Matter and Evolutions of Galaxies 2011
dc.sourceAIP Conference Proceedings
dc.subjectKeywords: Abundances; Nucleosynthesis; Stars: Abundances; Stars: AGB and Post-AGB
dc.titleCarbon-enhanced metal-poor stars and the s/r process
dc.typeConference paper
local.bibliographicCitation.lastpage116
local.bibliographicCitation.startpage111
local.contributor.affiliationLugaro, Maria, Monash University
local.contributor.affiliationKarakas, Amanda, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationStancliffe, Richard , College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationRijs, Carlos, Monash University
local.contributor.authoruidKarakas, Amanda, u4382192
local.contributor.authoruidStancliffe, Richard , u5083819
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB2778
local.identifier.doi10.1063/1.4763382
local.identifier.scopusID2-s2.0-84874511362
local.identifier.thomsonID000312157700019
local.type.statusPublished Version

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