Carbon-enhanced metal-poor stars: witnesses of the first generation of stars

Details Carbon-enhanced metal-poor stars: witnesses of the first generation of stars Carbon-enhanced metal-poor stars: witnesses of the first generation of stars

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sf2a.conf..321m&link_type=abstract

SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem,

Astronomy and Astrophysics

Astrophysics

Carbon Stars, Metal-Poor, Abundances

Scientific paper

Carbon-enhanced metal-poor (CEMP) stars are now accepted to be
mass-transferred binary member of the first generation of stars. Indeed,
the peculiar chemical fingerprints revealed by their spectra represent a
unique opportunity to study their now extinct progenitor (basically all
low-metallicity stars with M>0.8M_&sun;).

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