The Stellar Population of NGC 3576

Details The Stellar Population of NGC 3576 The Stellar Population of NGC 3576

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..267..359d&link_type=abstract

Hot Star Workshop III: The Earliest Stages of Massive Star Birth. ASP Conference Proceedings, Vol. 267. Edited by Paul A. Crowth

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Scientific paper

NGC3576 is a luminous HII region in the Carina arm, powered by a very young and massive star cluster. The most luminous members (probably O-type star progenitors) are still enshrouded in their natal cocoon. Some of those objects display CO in emission or absorption, a signature of accretion disks around YSOs. The luminosity function is similar to those found in other young clusters, suggesting a universal IMF through our Galaxy.

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