Carbon-rich, Extremely Metal-Poor Population II stars

dc.contributor.author	Ryan, Sean G.
dc.date.accessioned	2008-02-01T11:35:29Z
dc.date.available	2008-02-01T11:35:29Z
dc.date.issued	2003
dc.identifier.citation	Ryan , 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.isbn	1-58381-153-2
dc.identifier.other	dspace: 2299/1508
dc.identifier.other	ORCID: /0000-0001-9069-5122/work/30501358
dc.identifier.uri	http://hdl.handle.net/2299/1508
dc.description	Original paper can be found at: http://www.astrosociety.org/pubs/cs/286.html--Copyright Astronomical Society of the Pacific
dc.description.abstract	A 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.format.extent	417963
dc.language.iso	eng
dc.publisher	Astronomical Society of the Pacific
dc.relation.ispartof	Procs of CNO in the universe
dc.title	Carbon-rich, Extremely Metal-Poor Population II stars	en
dc.contributor.institution	Centre for Astrophysics Research (CAR)
dc.contributor.institution	School of Physics, Engineering & Computer Science
dc.contributor.institution	Department of Physics, Astronomy and Mathematics
rioxxterms.type	Other
herts.preservation.rarelyaccessed	true