Empirical calibration of the near-IR Ca II triplet - II. The stellar atmospheric parameters

Details Empirical calibration of the near-IR Ca II triplet - II. The stellar atmospheric parameters Empirical calibration of the near-IR Ca II triplet - II. The stellar atmospheric parameters

2001-09-10

arxiv.org/abs/astro-ph/0109158v1

Mon.Not.Roy.Astron.Soc. 326 (2001) 981

Astronomy and Astrophysics

Astrophysics

16 pages, 5 figures, LaTeX. For associated tables see http://www.ucm.es/info/Astrof/ellipt/CATRIPLET.html or http://www.nott

Scientific paper

10.1046/j.1365-8711.2001.04689.x

We present an homogeneous set of stellar atmospheric parameters (Teff, log g, [Fe/H]) for a sample of about 700 field and cluster stars which constitute a new stellar library in the near-infrared developed for stellar population synthesis in this spectral region (8350-9020 Angstrom). Having compiled the available atmospheric data in the literature for field stars, we have found systematic deviations between the atmospheric parameters from different bibliographic references. The Soubiran, Katz & Cayrel (1998) sample of stars with very well determined fundamental parameters has been taken as our standard reference system, and other papers have been calibrated and bootstrapped against it. The obtained transformations are provided in this paper. Once most of the datasets were on the same system, final parameters were derived by performing error weighted means. Atmospheric parameters for cluster stars have also been revised and updated according to recent metallicity scales and colour-temperature relations.

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