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dc.contributor.authorTsangarides, S.
dc.contributor.authorRyan, Sean G.
dc.contributor.authorBeers, T.C.
dc.date.accessioned2008-06-27T14:15:04Z
dc.date.available2008-06-27T14:15:04Z
dc.date.issued2003
dc.identifier.citationTsangarides , S , Ryan , S G & Beers , T C 2003 , Abundances and Kinematics of Extremely Metal-Deficient, Carbon-Rich Halo Stars . in Procs of CNO in the Universe : ASP Conf Series 304 . Astronomical Society of the Pacific , pp. 133-136 .
dc.identifier.isbn978-1-58381-637-0
dc.identifier.isbn1-58381-153-2
dc.identifier.otherdspace: 2299/2150
dc.identifier.otherORCID: /0000-0001-9069-5122/work/30501359
dc.identifier.urihttp://hdl.handle.net/2299/2150
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/286.html Copyright ASP
dc.description.abstractTo study the possible nucleosynthetic backgrounds of extremely metal-deficient, carbon-rich (EMDC) stars, we have conducted high-resolution spectroscopy of 26 candidate objects selected from HK-survey stars with [Fe/H]? -2.0. The aims of the analysis are: (a) to calculate abundances for the targets, including the CNO- and neutron-capture elements; (b) to monitor the radial velocities of the survey targets and another 17 bona fide EMDC stars to search for binarity.en
dc.format.extent326739
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofProcs of CNO in the Universe
dc.titleAbundances and Kinematics of Extremely Metal-Deficient, Carbon-Rich Halo Starsen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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