Nucleosynthesis on the Asymptotic Giant Branch: A comparison between codes

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dc.contributor.authorStancliffe, R J
dc.contributor.authorLugaro, Maria A
dc.contributor.authorKarakas, Amanda
dc.contributor.authorTout, Christopher A
dc.date.accessioned2015-12-07T22:46:37Z
dc.date.issued2005
dc.date.updated2015-12-07T11:43:48Z
dc.description.abstractWe present calculations of the thermally pulsing asymptotic giant branch (TP-AGB) phase of stellar evolution made with the fully implicit STARS code. These are the first detailed evolution calculations of the AGB phase to be made in this manner. Prelimi-
dc.identifier.issn0375-9474
dc.identifier.urihttp://hdl.handle.net/1885/25855
dc.publisherElsevier
dc.sourceNuclear Physics A
dc.titleNucleosynthesis on the Asymptotic Giant Branch: A comparison between codes
dc.typeJournal article
local.bibliographicCitation.lastpage572
local.bibliographicCitation.startpage569
local.contributor.affiliationStancliffe, R J, University of Cambridge
local.contributor.affiliationLugaro, Maria A, University of Cambridge
local.contributor.affiliationKarakas, Amanda, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationTout, Christopher A, University of Cambridge
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.ariespublicationu3379551xPUB41
local.identifier.citationvolume758
local.identifier.doi10.1016/j.nuclphysa.2005.05.105
local.identifier.scopusID2-s2.0-20944449457
local.type.statusPublished Version

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