Detection of Lead in the Carbon-rich, Very Metal-poor Star LP 625-44: A Strong Constraint on s-Process Nucleosynthesis at Low Metallicity

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dc.contributor.authorAoki, Wako
dc.contributor.authorNorris, John
dc.contributor.authorRyan, Sean G
dc.contributor.authorBeers, Timothy C
dc.contributor.authorAnderson, W G
dc.date.accessioned2015-12-13T23:18:48Z
dc.date.available2015-12-13T23:18:48Z
dc.date.issued2000
dc.date.updated2015-12-12T08:58:20Z
dc.description.abstractWe report the detection of the Pb I λ4057.8 line in the very metal-poor ([Fe/H] = -2.7), carbon-rich star, LP 625-44. We determine the abundance of Pb ([Pb/Fe] = 2.65) and 15 other neutron-capture elements. The abundance pattern between Ba and Pb agrees
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/90357
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Nuclear reactions; Nucleosynthesis; Stars: Abundances; Stars: AGB and post-AGB; Stars: Carbon; Stars: Population II
dc.titleDetection of Lead in the Carbon-rich, Very Metal-poor Star LP 625-44: A Strong Constraint on s-Process Nucleosynthesis at Low Metallicity
dc.typeJournal article
local.bibliographicCitation.lastpageL100
local.bibliographicCitation.startpageL97
local.contributor.affiliationAoki, Wako, National Astronomical Observatory of Japan
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.affiliationAnderson, W G, University of Texas
local.contributor.authoruidNorris, John, u7401084
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub20697
local.identifier.citationvolume536
local.identifier.scopusID2-s2.0-0034690833
local.type.statusPublished Version

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