High Mass Star Forming Gas in Cygnus X: The Molecular and Spitzer View of the DR21 Region

Details High Mass Star Forming Gas in Cygnus X: The Molecular and Spitzer View of the DR21 Region High Mass Star Forming Gas in Cygnus X: The Molecular and Spitzer View of the DR21 Region

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..357..153s&link_type=abstract

The Spitzer Space Telescope: New Views of the Cosmos ASP Conference Series, Volume 357, proceedings of the conference held 9-12

Astronomy and Astrophysics

Astronomy

Scientific paper

In order to study the processes by which rich clusters and high-mass stars form and evolve, we started a large scale molecular line and mm-continuum survey of Cygnus X, one of the richest and most active regions of our Galaxy. From this ongoing survey, we use molecular line observations (FCRAO, IRAM 30m) to investigate the relationship between molecular gas and the dust as seen in recently published IRAC and MIPS data of the DR21/W75 region.

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