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

Karakas, Amanda; Lattanzio, John

Description

The 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.contributor.authorKarakas, Amanda
dc.contributor.authorLattanzio, John
dc.date.accessioned2015-12-13T22:34:16Z
dc.identifier.issn1323-3580
dc.identifier.urihttp://hdl.handle.net/1885/76046
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.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.description.notesImported from ARIES
local.identifier.citationvolume31
dc.date.issued2014
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationU3488905xPUB4955
local.type.statusPublished Version
local.contributor.affiliationKarakas, Amanda, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLattanzio, John, Monash University
local.description.embargo2037-12-31
local.bibliographicCitation.issue12
local.bibliographicCitation.startpage62
local.identifier.doi10.1017/pasa.2014.21
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
dc.date.updated2015-12-11T09:19:34Z
local.identifier.scopusID2-s2.0-84910139196
local.identifier.thomsonID000339715200001
CollectionsANU Research Publications

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