Carbon abundances of three carbon-enhanced metal-poor stars from high-resolution Gemini-S/bHROS spectra of the ?8727 [C I] line

dc.contributor.authorSchuler, S. C.
dc.contributor.authorMergheim, S J
dc.contributor.authorSivarani, T
dc.contributor.authorAsplund, Martin
dc.contributor.authorSmith, Verne V
dc.contributor.authorCunha, Katia
dc.contributor.authorBeers, Timothy C
dc.date.accessioned2015-12-13T22:55:26Z
dc.date.issued2008
dc.date.updated2016-02-24T08:37:13Z
dc.description.abstractWe present the results from an analysis of the λ8727 forbidden [C I] line in high-resolution Gemini-S/bHROS spectra of three Carbon-Enhanced Metal-Poor (CEMP) stars. Previous derivations of C abundances in CEMP stars have primarily used the blue bands of
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/82527
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.subjectKeywords: stars: abundances; Stars: atmospheres; Stars: carbon; Stars: individual (HE 0054-2542, HE 0507-1653, HE 1005-1439); Stars: Population II
dc.titleCarbon abundances of three carbon-enhanced metal-poor stars from high-resolution Gemini-S/bHROS spectra of the ?8727 [C I] line
dc.typeJournal article
local.bibliographicCitation.issue6
local.bibliographicCitation.lastpage2258
local.bibliographicCitation.startpage2244
local.contributor.affiliationSchuler, S. C., National Optical Astronomy Observatory
local.contributor.affiliationMergheim, S J, Gemini Observatory
local.contributor.affiliationSivarani, T, Michigan State University
local.contributor.affiliationAsplund, Martin, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSmith, Verne V, National Optical Astronomy Observatory
local.contributor.affiliationCunha, Katia, Observatorio Nacional
local.contributor.affiliationBeers, Timothy C, Michigan State University
local.contributor.authoruidAsplund, Martin, u4042723
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB10787
local.identifier.citationvolume136
local.identifier.doi10.1088/0004-6256/136/6/2244
local.identifier.scopusID2-s2.0-66549112584
local.identifier.thomsonID000261042500004
local.type.statusPublished Version

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