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Evolution and nucleosynthesis of extremely metal-poor and metal-free low- and intermediate-mass stars. II. s-process nucleosynthesis during the core He flash

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Campbell, Simon; Lugaro, Maria; Karakas, Amanda

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Methods. We perform post-process nucleosynthesis calculations on a one-dimensional stellar evolution calculation of a star with mass 1 M· and a metallicity of [Fe/H] =-6.5 that suffers a proton ingestion episode. Our network includes 320 nuclear species

dc.contributor.authorCampbell, Simon
dc.contributor.authorLugaro, Maria
dc.contributor.authorKarakas, Amanda
dc.date.accessioned2015-12-08T22:44:27Z
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/37433
dc.description.abstractMethods. We perform post-process nucleosynthesis calculations on a one-dimensional stellar evolution calculation of a star with mass 1 M· and a metallicity of [Fe/H] =-6.5 that suffers a proton ingestion episode. Our network includes 320 nuclear species
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.titleEvolution and nucleosynthesis of extremely metal-poor and metal-free low- and intermediate-mass stars. II. s-process nucleosynthesis during the core He flash
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume522
dc.date.issued2010
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu3356449xPUB149
local.type.statusPublished Version
local.contributor.affiliationCampbell, Simon, Universitat Politécnica de Catalunya
local.contributor.affiliationLugaro, Maria, Monash University
local.contributor.affiliationKarakas, Amanda, College of Physical and Mathematical Sciences, ANU
local.description.embargo2037-12-31
local.bibliographicCitation.issue3
local.bibliographicCitation.startpage4
local.identifier.doi10.1051/0004-6361/201015428
dc.date.updated2015-12-08T10:45:04Z
local.identifier.scopusID2-s2.0-84887502221
local.identifier.thomsonID000284153100006
CollectionsANU Research Publications

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