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Carbon-enhanced metal-poor stars in the early galaxy

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dc.contributor.authorMarstellar, B
dc.contributor.authorBeers, Timothy C
dc.contributor.authorRossi, Silvia
dc.contributor.authorChristlieb, Norbert
dc.contributor.authorBessell, Michael
dc.contributor.authorRhee, Jaehyon
dc.date.accessioned2015-12-13T23:02:12Z
dc.date.issued2005
dc.date.updated2015-12-12T07:45:34Z
dc.description.abstractVery metal-deficient stars that exhibit enhancements of their carbon abundances are of crucial importance for understanding a number of issues - the nature of stellar evolution among the first generations of stars, the shape of the Initial Mass Function,
dc.identifier.issn0375-9474
dc.identifier.urihttp://hdl.handle.net/1885/84778
dc.publisherElsevier
dc.sourceNuclear Physics A
dc.titleCarbon-enhanced metal-poor stars in the early galaxy
dc.typeJournal article
local.bibliographicCitation.lastpage315c
local.bibliographicCitation.startpage312c
local.contributor.affiliationMarstellar, B, Michigan State University
local.contributor.affiliationBeers, Timothy C, Michigan State University
local.contributor.affiliationRossi, Silvia, Universidade de Sao Paulo
local.contributor.affiliationChristlieb, Norbert, University of Hamburg
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationRhee, Jaehyon, Yonsei University
local.contributor.authoruidBessell, Michael, u6900904
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub13023
local.identifier.citationvolume758
local.identifier.doi10.1016/j.nuclphysa.2005.05.056
local.identifier.scopusID2-s2.0-20944444585
local.type.statusPublished Version

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