An updated catalog of M33 clusters and candidates: photometry, and some statistical results
arXiv:1205.4822 · doi:10.1088/0004-6256/144/2/41
Abstract
We present photometry for 392 star clusters and candidates in the field of M33, which are selected from the most recent star cluster catalog. In this catalog, the authors listed star clusters' parameters such as cluster positions, magnitudes and colors in the filters, and so on. However, a large fraction of objects in this catalog do not have previously published photometry. Photometry is performed using archival images from the Local Group Galaxies Survey, which covers 0.8 deg along the major axis of M33. Detailed comparisons show that, in general, our photometry is consistent with previous measurements. Positions (right ascension and declination) for some clusters are corrected here. Combined with previous literature, we constitute a large sample of M33 star clusters. Based on this cluster sample, we present some statistical results: none of the M33 youngest clusters ( yr) have masses approaching ; roughly half the star clusters are consistent with the to mass models; the continuous distribution of star clusters along the model line indicates that M33 star clusters have been formed continuously from the epoch of the first star cluster formation until recent times; there are star clusters which being overlapped with the Galactic globular clusters on the color-color diagram, and these clusters are old globular clusters candidates in M33.
Accepted for Publication in AJ, 22 pages, 12 figures and 9 tables
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- The outer halo globular cluster system of M31 - III. Relationship to the stellar halo
- Deriving physical parameters of unresolved star clusters. I. Age, mass, and extinction degeneracies
- Star clusters in M33: updated UBVRI photometry, ages, metallicities, and masses
- Deriving physical parameters of unresolved star clusters IV. The M33 star cluster system
- New photometry of 234 M33 star clusters
- Structural Parameters for 10 Halo Globular Clusters in M33
- ACA CO(J=2-1) Mapping of the Nearest Spiral Galaxy M33. II. Exploring the Evolution of Giant Molecular Clouds