Carbon-rich, extremely metal-poor Population II stars

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dc.creatorRyan, Sean G.
dc.date2002-11-27
dc.date.accessioned2026-07-07T02:06:35Z
dc.date.available2026-07-07T02:06:35Z
dc.descriptionA 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.
dc.description4 pages including 1 figure. Conference proceedings for "CNO in the Universe", St Luc, Switzerland, 10-14 September 2002 C. Charbonnel, D. Schaerer & G. Meynet (eds) ASP Conference Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0211608
dc.identifierhttp://arxiv.org/abs/astro-ph/0211608
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5409
dc.subjectAstrophysics
dc.titleCarbon-rich, extremely metal-poor Population II stars
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