A&A 378, 97-101 (2001)
DOI: 10.1051/0004-6361:20011173
The self-enrichment of galactic halo globular clusters
The mass-metallicity relation
G. Parmentier1, 2 and G. Gilmore21 Institute of Astrophysics and Geophysics, University of Liège, avenue de Cointe 5, 4000 Liège, Belgium
2 Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK
(Received 10 July 2001 / Accepted 16 August 2001 )
Abstract
We discuss the existence
of a mass-metallicity relation among galactic
halo globular clusters. The lack of any luminosity-metallicity
correlation in globular cluster systems
has been used as an argument against
self-enrichment models of cluster formation.
We show that such a
relation is statistically present among the galactic Old Halo
globulars.
This observational correlation implies that the
least massive old clusters are the most metal-rich.
This is in contradiction with the idea
that, if globular clusters were self-enriched systems,
the most metal-rich clusters would also be the most massive
ones. We further show that this anti-correlation
is as predicted by self-enrichment models.
Key words: Galaxy: evolution -- Galaxy: formation -- globular clusters: general -- Galaxy: halo
Offprint request: G. Parmentier, parmentier@astro.ulg.ac.be
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