Extragalactic Globular Clusters. IV. The Data

Details Extragalactic Globular Clusters. IV. The Data Extragalactic Globular Clusters. IV. The Data

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apjs..102...29h&link_type=abstract

Astrophysical Journal Supplement v.102, p.29

Astronomy and Astrophysics

Astronomy

26

Galaxies: Stellar Content, Galaxy: Globular Clusters: General, Stars: Abundances

Scientific paper

We have explored the use of absorption line strength indices, measured from integrated globular cluster spectra, to predict mean metallicity in late-type stellar systems. In previous papers we identified the best indices for such metallicity calibrations out of ~13 measured in a large sample of galactic and M31 cluster spectra. In this paper we present the individual measurements of 13 indices and averages of multiple measurements, where appropriate. Data are given for 151 M31 globular clusters, 88 galaxies, 22 M33 cluster candidates, 10 M87 clusters, eight M81 globular clusters, three Fornax dwarf galaxy clusters, "standard" stars from the lists of Faber et al., stars in the open cluster NGC 188 and, for completeness, other stars observed as candidate globular clusters.

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