Evolution of [O/Mg], [Na/Mg], [Al/Mg], and [K/Mg] in the Galaxy, from a NLTE analysis

Details Evolution of [O/Mg], [Na/Mg], [Al/Mg], and [K/Mg] in the Galaxy, from a NLTE analysis Evolution of [O/Mg], [Na/Mg], [Al/Mg], and [K/Mg] in the Galaxy, from a NLTE analysis

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..265..380s&link_type=abstract

Chemical Abundances in the Universe: Connecting First Stars to Planets, Proceedings of the International Astronomical Union, IAU

Astronomy and Astrophysics

Astronomy

2

Abundances, Line:Profiles, Pop Ii, Halo

Scientific paper

In the framework of he ESO Large Program “First Stars”, high
resolution (R=45000) high S/N ratio spectra have been obtained for a
sample of Extremely Metal Poor Stars (EMP stars), 35 giants and 18
turnoff stars. Among them 37 have a very low metallicity: [Fe/H]<
-2.9.

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