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The Circumstellar Environment of Low Mass Star Forming RegionsWe have obtained the complete SED from 10 microns out to 1.3 mm for all of our sources. We have the FIR imaging data, processed to reveal the maximum angular resolution possible, which allows us to model the disk. To model the disk, we have high resolution millimeter interferometry data.
Document ID
19970028299
Acquisition Source
Ames Research Center
Document Type
Contractor Report (CR)
Authors
Butner, Harold M. (Carnegie Institution of Washington Pasadena, CA United States)
Date Acquired
September 6, 2013
Publication Date
June 5, 1997
Subject Category
Astronomy
Report/Patent Number
NASA-CR-204638
NAS 1.26:204638
Accession Number
97N27089
Funding Number(s)
CONTRACT_GRANT: NAG2-959
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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