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Massive Quiescent Cores in Orion - The Core Mass FunctionCMF studies to date have been largely restricted to low-mass star-forming regions. The present study focuses on a HIGH MASS star forming region, ORION, but observes positions sufficiently far from KL that effects of previously-formed massive stars are not overwhelming
Document ID
20060051748
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
hdl:2014/39763
Authors
Li, Di (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Goldsmith, Paul F. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Velusamy, Thangasamy (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Langer, Bill (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 23, 2013
Publication Date
January 1, 2006
Subject Category
Astronomy
Meeting Information
Meeting: Cornell Caltech Atacama Telescope Project Meeting
Location: Ithaca, NY
Country: United States
Start Date: July 19, 2006
Distribution Limits
Public
Copyright
Other
Keywords
molecular cloud cores
star fomation

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