Physics
Scientific paper
Nov 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35369071j&link_type=abstract
VizieR On-line Data Catalog: J/A+A/536/A71. Originally published in: 2011A&A...536A..71J
Physics
Stars: Giant, Abundances: [Fe/H], Rotational Velocities, Spectroscopy
Scientific paper
We used high resolution and high S/N spectra to measure the equivalent widths of many FeI and FeII lines, which were used to derive the atmospheric parameters by imposing local thermodynamic and ionization equilibrium. The effective temperatures and metallicities were used, along with stellar evolutionary tracks to determine the physical properties and evolutionary status of each star.
(1 data file).
Jenkins James S.
Jones Matias I.
Melo H. F. C.
Rojo Patricio
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