Dense Molecular Gas Clumps Associated with Clustered Star Formation in the Rosette Molecular Cloud

Details Dense Molecular Gas Clumps Associated with Clustered Star Formation in the Rosette Molecular Cloud Dense Molecular Gas Clumps Associated with Clustered Star Formation in the Rosette Molecular Cloud

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..206r&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

Ism: Molecules, Molecular Clouds, Radio Lines: Ism, Stars: Formation

Scientific paper

Millimeter-wavelength observations of molecular clumps play a crucial role in understanding the process of clustered star formation in giant molecular clouds. The morphology and chemistry of molecular material around embedded clusters defined by tracers of dense gas, allow us to describe the interaction between the newly born stars and the remnants of the condensations from which they hatched.

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