Cepheid Mass loss and the Pulsation-Evolutionary Mass Discrepancy

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dc.contributor.authorKeller, Stefan
dc.date.accessioned2015-12-08T22:25:13Z
dc.date.issued2008
dc.date.updated2015-12-08T09:03:59Z
dc.description.abstractI investigate the discrepancy between the evolution and pulsation masses for Cepheid variables. A number of recent works have proposed that noncanonical mass loss can account for the mass discrepancy. This mass loss would be such that a 5 M·, star loses
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/33348
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Cepheids; Stars: evolution; Stars: oscillations (including pulsations)
dc.titleCepheid Mass loss and the Pulsation-Evolutionary Mass Discrepancy
dc.typeJournal article
local.bibliographicCitation.issueApril
local.bibliographicCitation.lastpage487
local.bibliographicCitation.startpage483
local.contributor.affiliationKeller, Stefan, College of Physical and Mathematical Sciences, ANU
local.contributor.authoremailrepository.admin@anu.edu.au
local.contributor.authoruidKeller, Stefan, u9702857
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4362859xPUB101
local.identifier.citationvolume677
local.identifier.doi10.1086/529366
local.identifier.scopusID2-s2.0-42549100442
local.identifier.thomsonID000254754300037
local.identifier.uidSubmittedByu4362859
local.type.statusPublished Version

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