Revealing the Galactic ``Underground'' Star Formation

Details Revealing the Galactic ``Underground'' Star Formation Revealing the Galactic ``Underground'' Star Formation

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009rmxac..35...54b&link_type=abstract

XII Latin American IAU Regional Meeting (Eds. G. Magris, G. Bruzual, & L. Carigi) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

1

Galaxy: Open Clusters And Associations, Infrared: General, Stars: Formation

Scientific paper

We are reporting some recent results from our long-term program aimed at better understanding of the hidden present-day star cluster population in the Galaxy. So far, most clusters from our studies have typical ages of 3-10 Myr, and typical masses of order of a few thousand solar masses. Only two of them -[DBSB2003] 179 and RCW 87- are moderately massive (at or approaching 10^4 solar masses).

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