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 | |