Carbon-enhanced metal-poor stars (Masseron+, 2010)

Details Carbon-enhanced metal-poor stars (Masseron+, 2010) Carbon-enhanced metal-poor stars (Masseron+, 2010)

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35099093m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/509/A93. Originally published in: 2010A&A...509A..93M

Computer Science

Stars: Population Ii, Stars: Metal-Deficient, Abundances

Scientific paper

We compiled abundances from analyses of high-resolution spectra (R>40000) of CEMP stars (Tables 1 and 2), Ba stars, and non-C-enhanced metal-poor stars (Tables 3 and 4). C-rich stars are defined as stars with [C/Fe]>0.9. In this paper, all plots are compiled exclusively of data from these tables, including our own data from Paper II (Masseron et al., in prep.). All these data are renormalised by the Asplund (2005ARA&A..43..481A) solar abundances.
(5 data files).

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