- ... 32
- Based on observations
collected at ESO telescopes under programs 072.D-0550 and 074.D-0571.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
- Tables 7, 9-11 are only available in electronic form at http://www.aanda.org
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... IRAF
- IRAF is distributed by the National Optical
Astronomical Observatories, which are operated by the Association of
Universities for Research in Astronomy, under contract with the National
Science Foundation.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
(2MASS
- The Two Micron All Sky Survey is a joint project of the
University of Massachusetts and the Infrared Processing and Analysis
Center/California Institute of Technology, funded by the national Aeronautics
and Space Administration and the National Science Foundation.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...1973)
- http://verdi.as.utexas.edu/
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... transitions
- MOOG was recently updated in order to give the
possibility of using the Barklem coefficients.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...

-
,
absolute number density abundance.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... literature
- Part of these data are collected in Table 7 of Friel
et al. (2003, see also references therein);
others are from Carretta et
al. (2004, 2005), Carraro et al. (2004),
Villanova et al. (2005), Yong et al. (2005), Randich et al. (2006), Gratton et al. (2006);
note that the quoted investigations are all based on
giant stars with the exception of Randich et al. (2006)
in which dwarfs
and slightly evolved stars of M 67 were considered.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
database
- http://www.univie.ac.at/webda/
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.