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Mg And Al production in intermediate-mass asymptotic giant branch stars

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dc.contributor.authorKarakas, Amanda
dc.contributor.authorLugaro, Maria Anna
dc.contributor.authorUgalde, C.
dc.contributor.authorWiescher, M.
dc.contributor.authorGörres, Joachim
dc.date.accessioned2015-12-07T22:49:32Z
dc.date.issued2006
dc.date.updated2015-12-07T12:09:20Z
dc.description.abstractWe study how the production of the magnesium and aluminum isotopes in intermediate mass Asymptotic Giant Branch stars is affected by uncertainties in the 22Ne + α-capture reaction rates. We use new estimates of these rates with smaller uncertainties comp
dc.identifier.issn1387-6473
dc.identifier.urihttp://hdl.handle.net/1885/26806
dc.publisherElsevier
dc.sourceNew Astronomy Reviews
dc.subjectKeywords: Abundances; Nucleosynthesis; Stars: AGB and post-AGB-nuclear reactions
dc.titleMg And Al production in intermediate-mass asymptotic giant branch stars
dc.typeJournal article
local.bibliographicCitation.issue7-8
local.bibliographicCitation.lastpage503
local.bibliographicCitation.startpage500
local.contributor.affiliationKarakas, Amanda, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLugaro, Maria Anna, Utrecht University
local.contributor.affiliationUgalde, C., University of North Carolina
local.contributor.affiliationWiescher, M., University of Notre Dame
local.contributor.affiliationGörres, Joachim, University of Notre Dame
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.ariespublicationu3379551xPUB47
local.identifier.citationvolume50
local.identifier.doi10.1016/j.newar.2006.06.013
local.identifier.scopusID2-s2.0-33749137075
local.type.statusPublished Version

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