Physics
Scientific paper
Sep 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..35059013g&link_type=abstract
VizieR On-line Data Catalog: J/A+A/505/L13. Originally published in: 2009A&A...505L..13G
Physics
Clusters: Globular, Stars: Dwarfs, Stars: Giant, Equivalent Widths, Effective Temperatures
Scientific paper
Photometric data of the dwarf and subgiant stars of the globular cluster NGC 6397. We also provide the signal-to-noise of the spectra, the 3D and 1D Halpha-based effective temperatures, 3D Li abundances, and the equivalent widths and errors: dEWa: Error of the equivalent width measurements estimated from a fitting routine that uses as free parameters the velocity shift, the continuum location, and the equivalent width of the Li line. dEWb: Error of the equivalent width associated to the signal-to-noise ratio and the wavelength dispersion of the spectra, derived using Cayrel's formula (Cayrel, 1988, IAU Symp. 132: The Impact of Very High S/N Spectroscopy on Stellar Physics, 132, 345).
(1 data file).
Behara N. T.
Bonifacio Piercarlo
Caffau Elisabetta
Cayrel Roger
Gonzalez Hernandez Jonay I.
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