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Far-infrared observations of W51 with high spatial resolutionObservations of the core of W51 have been made from the NASA C-141 Airborne Infrared Observatory at 55 microns with 17-, 35-, and 85-arc sec apertures and at 100 microns with a 35-arc sec aperture. These observations suggest the presence of a small less than about 20 arc sec source at 55 microns surrounded by a much broader diffuse background. In the center of the source the optical depth at 55 and 100 microns is on the order of 0.1-0.2.
Document ID
19750040260
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Harvey, P. M.
Hoffmann, W. F.
Campbell, M. F.
(Steward Observatory Tucson, Ariz., United States)
Date Acquired
August 8, 2013
Publication Date
February 15, 1975
Publication Information
Publication: Astrophysical Journal
Volume: 196
Subject Category
Astrophysics
Accession Number
75A24332
Funding Number(s)
CONTRACT_GRANT: NGR-03-002-390
Distribution Limits
Public
Copyright
Other

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