NGC6397 red giants chemical composition (Lind+, 2011)

Details NGC6397 red giants chemical composition (Lind+, 2011) NGC6397 red giants chemical composition (Lind+, 2011)

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35279148l&link_type=abstract

VizieR On-line Data Catalog: J/A+A/527/A148. Originally published in: 2011A&A...527A.148L

Physics

Clusters: Globular, Abundances, Equivalent Widths

Scientific paper

The tables contain stellar parameters, equivalent widths, and line-by-line abundances for stars in the metal-poor globular cluster NGC6397. All abundances are given in logarithmic units relative to hydrogen, according to A(x)=log(N(x)/N(H))+12, where N(x) is the number density of element x and N(H) the number density of hydrogen. For photometric data, Li abundances, and equivalent widths of Fe lines we refer to Lind et al. (2009, Cat. J/A+A/503/545). Table 2 contains improved non-LTE Na abundances for the targets presented in Lind et al (2009,, Cat. J/A+A/503/545).
(2 data files).

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