Low-mass X-ray Binaries and Globular Clusters in Early-type Galaxies. Ii. Globular Cluster Candidates and Their Mass-metallicity Relation

We present an astrometry and photometry catalogue of globular cluster (GC) candidates detected with HST WFPC2 in a sample of 19 early-type galaxies, appropriate for comparison to the lowmass X-ray binary (LMXB) populations observed with Chandra. In a companion paper, we present the Chandra data and investigate the relation between these populations. We demonstrate that, although there is little evidence of a colour-magnitude correlation for the GCs, after estimating mass and metallicity from the photometry, under the assumption of a single age simple stellar population, there is a significant positive correlation between mass and metallicity. We constrained [Z/H] = (−2.1± 0.2) + (0.25± 0.04)log10M, with a 1-σ intrinsic scatter of 0.62 dex in metallicity. If GCs are bimodal in metallicity this relation is consistent with recent suggestions of a mass-metallicity relation only for metal-poor clusters. Adopting a new technique to fit the GC luminosity function (GCLF) accounting for incompleteness and the Eddington bias, we compute the V-band local GC specific frequency (SN) and specific luminosity (SL) of each galaxy. We show that SL is the more robust measure of the richness of a GC population where a significant fraction is undetected due to source detection incompleteness. We find that the absolute magnitude of the GCLF turnover exhibits intrinsic scatter from galaxy to galaxy of ∼0.3 mag (1-σ), limiting its accuracy as a standard distance measure. Subject headings: galaxies: elliptical and lenticular, cD— galaxies: star clusters— galaxies: general— galaxies: distances and redshifts