Extremely Metal-poor Stars. IX. CS 22949-037 and the Role of Hypernovae

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dc.contributor.authorNorris, John
dc.contributor.authorRyan, Sean G
dc.contributor.authorBeers, Timothy C
dc.contributor.authorAoki, Wako
dc.contributor.authorAnderson, W G
dc.date.accessioned2015-12-13T22:30:55Z
dc.date.available2015-12-13T22:30:55Z
dc.date.issued2002
dc.date.updated2015-12-11T08:57:53Z
dc.description.abstractWe have obtained high-resolution spectra of the extremely metal-poor star CS 22949-037 ([Fe/H] = -3.79) in the region of the ultraviolet NH bands at 3360-3370 Å, which confirm our earlier report that it exhibits extreme nitrogen enhancement. We find [N/F
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/75057
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: Population II
dc.titleExtremely Metal-poor Stars. IX. CS 22949-037 and the Role of Hypernovae
dc.typeJournal article
local.bibliographicCitation.lastpageL110
local.bibliographicCitation.startpageL107
local.contributor.affiliationNorris, John, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationRyan, Sean G, Open University
local.contributor.affiliationBeers, Timothy C, Michigan State University
local.contributor.affiliationAoki, Wako, National Astronomical Observatory of Japan
local.contributor.affiliationAnderson, W G, University of Texas
local.contributor.authoremailu7401084@anu.edu.au
local.contributor.authoruidNorris, John, u7401084
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub4445
local.identifier.citationvolume569
local.identifier.doi10.1086/340665
local.identifier.scopusID2-s2.0-0000982915
local.identifier.uidSubmittedByMigrated
local.type.statusPublished Version

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