The Lick Fe5015, Fe5270, Fe5335, Mgb and Mg2 indices are presented for 139 candidate SMR stars of different luminosity class studied in Malagnini et al. (2000). Evidence is found for a standard (i.e. [Mg/Fe]~0) Mg vs. Fe relative abundance. Both the Worthey et al. (1994) and Buzzoni et al. (1992, 1994) fitting functions are found to suitably match the data at super-solar metallicity regimes. See http://www.merate.mi.astro.it/~eps/home.html for further details.
@article{arxiv.astro-ph/0109443,
title = {Lick Spectral Indices for Super Metal-rich Stars},
author = {A. Buzzoni and M. Chavez and M. L. Malagnini and C. Morossi},
journal= {arXiv preprint arXiv:astro-ph/0109443},
year = {2009}
}
Comments
16 pages with 11 figures (Aastex format). To appear in the Nov. '01 issue of the PASP