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The galaxy's 157 micron (C 2) emission: Observations by means of a spectroscopic lunar-occultation techniqueGalactic (C II) 157 micron, fine-structure emission was estimated. At a Galactic longitude of 8 deg, the peak power observed in a 7' x 7' field is approx. 5 x 10 to the -9 Watt. The method used to detect this radiation involved chopping against the cold side of the Moon.
Document ID
19830016166
Acquisition Source
Legacy CDMS
Document Type
Preprint (Draft being sent to journal)
Authors
Stacey, G. J. (NASA Ames Research Center Moffett Field, CA, United States)
Smyers, S. D. (NASA Ames Research Center Moffett Field, CA, United States)
Kurtz, N. T. (NASA Ames Research Center Moffett Field, CA, United States)
Harwit, M. (NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
September 4, 2013
Publication Date
April 1, 1983
Subject Category
Astronomy
Report/Patent Number
NASA-TM-84355
NAS 1.15:84355
A-9312
Report Number: NASA-TM-84355
Report Number: NAS 1.15:84355
Report Number: A-9312
Accession Number
83N24437
Funding Number(s)
PROJECT: RTOP 352-02-03
CONTRACT_GRANT: NGR-33-010-146
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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