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dc.contributor.authorRyan, Sean G.
dc.date.accessioned2008-02-01T11:35:29Z
dc.date.available2008-02-01T11:35:29Z
dc.date.issued2003
dc.identifier.citationRyan , S G 2003 , Carbon-rich, Extremely Metal-Poor Population II stars . in Procs of CNO in the universe : ASP Conf Series 304 . Astronomical Society of the Pacific , pp. 128-132 .
dc.identifier.isbn1-58381-153-2
dc.identifier.otherPURE: 143772
dc.identifier.otherPURE UUID: 661262c6-30e8-4d6e-8e4f-febb76723446
dc.identifier.otherdspace: 2299/1508
dc.identifier.otherORCID: /0000-0001-9069-5122/work/30501358
dc.identifier.urihttp://hdl.handle.net/2299/1508
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/286.html--Copyright Astronomical Society of the Pacific
dc.description.abstractA significant fraction of very metal-poor stars have unexpectedly high carbon abundances. I recap on their discovery, describe the results of high-resolution spectroscopic studies of their composition, and consider possible origins. It is now clear that at least two, and possibly three different explanations are needed for their general characteristics.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofProcs of CNO in the universe
dc.titleCarbon-rich, Extremely Metal-Poor Population II starsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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