Young Star Clusters in M 31

@inproceedings{Morrison2008YoungSC,
  title={Young Star Clusters in M 31},
  author={Heather L. Morrison and Nelson Caldwell and Paul Harding and Jeffrey Robert Kriessler and James A. Rose and Ricardo P. Schiavon},
  year={2008}
}
In our study of M 31’s globular cluster system with MMT/Hectospec, we have obtained high-quality spectra of 85 clusters with ages less than 1 Gyr. With the exception of Hubble V, the young cluster in NGC 205, we find that these young clusters have kinematics and spatial distribution consistent with membership in M 31’s young disk. Preliminary estimates of the cluster masses and structural parameters, using spectroscopically derived ages and HST imaging, confirms earlier suggestions that M 31… 

References

SHOWING 1-10 OF 18 REFERENCES
PROPERTIES OF YOUNG STAR CLUSTERS IN M 31.
Integrated UBVR photometry is given for a selection of young star clusters and compact OB associations in M31. Most are very young and, except for those in the outer parts of the galaxy, most show
Identification and Analysis of Young Star Cluster Candidates in M31
We present a method for finding clusters of young stars in M31 using broadband WFPC2 data from the HST data archive. Applying our identification method to 13 WFPC2 fields, covering an area of ~60
Massive Young Clusters in the Disk of M31
We have studied the properties of a sample of 67 very blue and likely young massive clusters in M31 extracted from the Bologna Revised Catalog of globular clusters, selected according to their color
Resolved Massive Star Clusters in the Milky Way and Its Satellites: Brightness Profiles and a Catalog of Fundamental Parameters
We present a database of structural and dynamical properties for 153 spatially resolved star clusters in the Milky Way, the Large and Small Magellanic Clouds, and the Fornax dwarf spheroidal. This
Astrophysical parameters of Galactic open clusters
We present a catalogue of astrophysical data for 520 Galactic open clusters. These are the clusters for which at least three most probable members (18 on average) could be identified in the ASCC-2.5,
Globular Cluster and Galaxy formation: M31, The Milky Way, and Implications for Globular Cluster Systems of Spiral Galaxies
We find that the globular cluster (GC) systems of the Milky Way and of our neighboring spiral galaxy, M31, comprise two distinct entities, differing in three respects. First, M31 has a set of young
Giant H II regions and the formation of populous star clusters
Published observational data on the populations of nearby giant H II regions (GHRs) and blue globular star clusters (BGCs) are compiled in tables and graphs and compared with the predictions of a
The Chemical Properties of Milky Way and M31 Globular Clusters. I. A Comparative Study
A comparative analysis is performed between high-quality integrated spectral indices of 30 M31 globular clusters, 20 Milky Way globular clusters, and a sample of field and cluster elliptical
On the massive stellar population of the super star cluster Westerlund 1
We present new spectroscopic and photometric observations of the young Galactic open cluster Westerlund 1 (Wd 1) that reveal a unique population of massive evolved stars. We identify ∼200 cluster
M31 Globular Clusters: Colors and Metallicities
We present a new catalog of photometric and spectroscopic data on M31 globular clusters (GCs). The catalog includes new optical and near-infrared photometry for a substantial fraction of the 435
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