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

TL;DR

This paper reports the discovery of the largest known cluster of Red Supergiants in the Milky Way, providing insights into massive star evolution, cluster mass, and Galactic structure at the interface of the disk and bulge.

Contribution

It identifies and characterizes a massive RSG cluster at the base of the Scutum-Crux arm, the largest known such cluster, and discusses its implications for Galactic evolution.

Findings

Largest known RSG cluster with 26 members

Cluster mass estimated at ~40,000 solar masses

Indications of recent starburst activity in the region

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.