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The Dawes Review 2: Nucleosynthesis and stellar yields of low-and intermediate-mass single stars

dc.contributor.authorKarakas, Amanda
dc.contributor.authorLattanzio, John
dc.date.accessioned2015-12-13T22:34:16Z
dc.date.issued2014
dc.date.updated2015-12-11T09:19:34Z
dc.description.abstractThe chemical evolution of the Universe is governed by the chemical yields from stars, which in turn are determined primarily by the initial stellar mass. Even stars as low as 0.9 M⊙ can, at low metallicity, contribute to the chemical evolution of elemen
dc.identifier.issn1323-3580
dc.identifier.urihttp://hdl.handle.net/1885/76046
dc.publisherCSLI Publications
dc.sourcePublications of the Astronomical Society of Australia
dc.titleThe Dawes Review 2: Nucleosynthesis and stellar yields of low-and intermediate-mass single stars
dc.typeJournal article
local.bibliographicCitation.issue12
local.bibliographicCitation.startpage62
local.contributor.affiliationKarakas, Amanda, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLattanzio, John, Monash University
local.contributor.authoruidKarakas, Amanda, u4382192
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationU3488905xPUB4955
local.identifier.citationvolume31
local.identifier.doi10.1017/pasa.2014.21
local.identifier.scopusID2-s2.0-84910139196
local.identifier.thomsonID000339715200001
local.type.statusPublished Version

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