Properties of Young Massive Clusters Derived from Spectroscopy

Details Properties of Young Massive Clusters Derived from Spectroscopy Properties of Young Massive Clusters Derived from Spectroscopy

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..322...81t&link_type=abstract

The Formation and Evolution of Massive Young Star Clusters, ASP Conference Series, Vol. 322. Edited by H.J.G.L.M. Lamers, L.J.

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Spectroscopy of young massive clusters is generally much more expensive in terms of telescope time than photometry. However, the return on this investment is generally high. In this review we consider the physical properties of young massive clusters which may be derived from UV, optical, and near-IR spectroscopy. We highlight various methods of constraining cluster age, metallicity, and reddening.

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