Star formation in young embedded clusters: New observational results using near-infrared detector arrays

Details Star formation in young embedded clusters: New observational results using near-infrared detector arrays Star formation in young embedded clusters: New observational results using near-infrared detector arrays

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994inpht..35..167h&link_type=abstract

Infrared Physics & Technology, Volume 35, Issue 2-3, p. 167-174.

Physics

Scientific paper

A significant fraction of all recently formed stars in the Galaxy are found in embedded groups and clusters of young stars. Infrared imaging, photometry, and spectroscopy can be used to study the evolutionary history of such young clusters. Initial observations indicate that star formation in clusters is going on for an extended time (~l06yr) with only a few stars in the main accretion phase at any given time.

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