Journal
ASTROPHYSICAL JOURNAL
Volume 733, Issue 1, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/733/1/41
Keywords
infrared: stars; stars: evolution
Categories
Funding
- ERC [GLOSTAR (247078)]
- NASA [NNG 05-GC37G]
- NYSTAR Faculty Development Program
- US National Science Foundation [AST-0709479]
- Alexander-von-Humboldt Foundation
- Spanish Ministerio de Ciencia e Innovacion [AYA2008-06166-C03-02]
- National Aeronautics and Space Administration
- NSF
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Young massive (M > 10(4)M(circle dot)) stellar clusters are a good laboratory to study the evolution of massive stars. Only a dozen of such clusters are known in the Galaxy. Here, we report about a new young massive stellar cluster in the Milky Way. Near-infrared medium-resolution spectroscopy with UIST on the UKIRT telescope and NIRSPEC on the Keck telescope, and X-ray observations with the Chandra and XMM satellites, of the Cl 1813-178 cluster confirm a large number of massive stars. We detected 1 red supergiant, 2 Wolf-Rayet stars, 1 candidate luminous blue variable, 2 OIf, and 19 OB stars. Among the latter, twelve are likely supergiants, four giants, and the faintest three dwarf stars. We detected post-main-sequence stars with masses between 25 and 100M(circle dot). A population with age of 4-4.5 Myr and a mass of similar to 10,000M(circle dot) can reproduce such a mixture of massive evolved stars. This massive stellar cluster is the first detection of a cluster in the W33 complex. Six supernova remnants and several other candidate clusters are found in the direction of the same complex.
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