A massive cluster of Red Supergiants at the base of the Scutum-Crux arm

Abstract

We report on the unprecedented Red Supergiant (RSG) population of a massive young cluster, located at the base of the Scutum-Crux Galactic arm. We identify candidate cluster RSGs based on {\it 2MASS} photometry and medium resolution spectroscopy. With follow-up high-resolution spectroscopy, we use CO-bandhead equivalent width and high-precision radial velocity measurements to identify a core grouping of 26 physically-associated RSGs -- the largest such cluster known to-date. Using the stars' velocity dispersion, and their inferred luminosities in conjuction with evolutionary models, we argue that the cluster has an initial mass of $\sim$40,000\msun, and is therefore among the most massive in the galaxy. Further, the cluster is only a few hundred parsecs away from the cluster of 14 RSGs recently reported by Figer et al (2006). These two RSG clusters represent 20% of all known RSGs in the Galaxy, and now offer the unique opportunity to study the pre-supernova evolution of massive stars, and the Blue- to Red-Supergiant ratio at uniform metallicity. We use GLIMPSE, MIPSGAL and MAGPIS survey data to identify several objects in the field of the larger cluster which seem to be indicative of recent region-wide starburst activity at the point where the Scutum-Crux arm intercepts the Galactic bulge. Future abundance studies of these clusters will therefore permit the study of the chemical evolution and metallicity gradient of the Galaxy in the region where the disk meets the bulge.

49 pages, 22 figures. Accepted for publication in ApJ. Version with hi-res figures can be found at http://www.cis.rit.edu/~bxdpci/RSGC2.pdf

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• Red supergiants around the obscured open cluster Stephenson 2
• Hyperfast pulsars as the remnants of massive stars ejected from young star clusters
• Discovery of a young massive stellar cluster near HESS J1813-178
• Massive Star Forming Regions in the Galaxy using the Spitzer GLIMPSE Survey
• The young Galactic star cluster [DBS2003]179
• The Discovery of a Massive Cluster of Red Supergiants with GLIMPSE
• Young Massive Clusters
• WR 120bb and WR 120bc: a pair of WN9h stars with possibly interacting circumstellar shells
• OB Associations at the Upper End of the Milky Way Luminosity Function