Equivalent widths of Li, Na, Fe, Ca in NGC 6397 (Lind+, 2009)

Details Equivalent widths of Li, Na, Fe, Ca in NGC 6397 (Lind+, 2009) Equivalent widths of Li, Na, Fe, Ca in NGC 6397 (Lind+, 2009)

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..35030545l&link_type=abstract

VizieR On-line Data Catalog: J/A+A/503/545. Originally published in: 2009A&A...503..545L

Physics

Atomic Physics

Clusters: Globular, Stars: Late-Type, Abundances, Atomic Physics

Scientific paper

The tables contain coordinates, photometry, derived stellar parameters, equivalent widths, and abundances for a large number of dwarfs, subgiant branch stars, and red giant branch 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. Table 3 contains only a subset (32) of all targets. The oscillator strengths adopted are listed in the paper.
(3 data files).

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