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Element Enhancements along the Entire Asymptotic Giant Branch Phase

Wylie de Boer, Elizabeth; Cottrell, P L

Description

The results of a study of the asymptotic giant branch (AGB) phase of stellar evolution are presented. Abundances have been determined for Fe, C, O, the light s-process elements, Y and Zr, the heavy s-process elements, La and Nd, and the r-process element,

dc.contributor.authorWylie de Boer, Elizabeth
dc.contributor.authorCottrell, P L
dc.date.accessioned2015-12-08T22:26:14Z
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/33600
dc.description.abstractThe results of a study of the asymptotic giant branch (AGB) phase of stellar evolution are presented. Abundances have been determined for Fe, C, O, the light s-process elements, Y and Zr, the heavy s-process elements, La and Nd, and the r-process element,
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: nuclear reactions, nucleosynthesis, abundances; stars: abundances; stars: AGB and post-AGB
dc.titleElement Enhancements along the Entire Asymptotic Giant Branch Phase
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume692
dc.date.issued2009
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu3356449xPUB104
local.type.statusPublished Version
local.contributor.affiliationWylie de Boer, Elizabeth, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationCottrell, P L, University of Canterbury
local.description.embargo2037-12-31
local.bibliographicCitation.issue1
local.bibliographicCitation.startpage522
local.bibliographicCitation.lastpage530
local.identifier.doi10.1088/0004-637X/692/1/522
dc.date.updated2016-02-24T09:53:30Z
local.identifier.scopusID2-s2.0-84876792235
local.identifier.thomsonID000263553000045
CollectionsANU Research Publications

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