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Evolutionary implications of the new triple-α nuclear reaction rate for low mass stars (Research Note)

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dc.contributor.authorDotter, Aaron
dc.contributor.authorPaxton, Bill
dc.date.accessioned2015-12-13T22:48:54Z
dc.date.issued2009
dc.date.updated2016-02-24T09:42:55Z
dc.description.abstractContext.Ogata et al. (2009, Progr. Theor. Phys., 122, 1055) presented a theoretical determination of the 4He(αα, γ)12C, or triple-α, nuclear reaction rate. Their rate differs from the NACRE rate by many orders of magnitude at temperatures relevant for
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/80276
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: C-M diagrams; Late stage; Low-mass stars; Nuclear reaction rates; Nuclear reactions , nucleosynthesis , abundances; Orders of magnitude; Red giant branches; Red giants; Stellar evolutions; Stellar models; Stellar system; Chemical elements; Helium; High en C-M diagrams; Nuclear reactions, nucleosynthesis, abundances; Stars: evolution; Stars: Hertsprung-Russell (HR)
dc.titleEvolutionary implications of the new triple-α nuclear reaction rate for low mass stars (Research Note)
dc.typeJournal article
local.bibliographicCitation.issue3
local.bibliographicCitation.lastpage1619
local.bibliographicCitation.startpage1617
local.contributor.affiliationDotter, Aaron, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationPaxton, Bill, University of California
local.contributor.authoruidDotter, Aaron, u5239381
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB8556
local.identifier.citationvolume507
local.identifier.doi10.1051/0004-6361/200912998
local.identifier.scopusID2-s2.0-70849084561
local.type.statusPublished Version

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