Fe Abundances in metal-poor stars (Sbordone+ 2010)

Details Fe Abundances in metal-poor stars (Sbordone+ 2010) Fe Abundances in metal-poor stars (Sbordone+ 2010)

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35229026s&link_type=abstract

VizieR On-line Data Catalog: J/A+A/522/A26. Originally published in: 2010A&A...522A..26S

Physics

Abundances: [Fe/H], Abundances: Peculiar, Stars: Population Ii

Scientific paper

Line-by-line abundances for FeI and FeII lines used to estimate metallicity and gravity for the program stars. The first column lists the star name, then the ion (FeI or FeII) The the wavelength in nm, the loggf, the measured EW (pm) and the derived abundance assuming the four stellar parameter sets used in the article, respectively 3D, BA, ALI and IRFM.
(3 data files).

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