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A high resolution far-infrared survey of a section of the galactic plane. II - Far-infrared, CO, and radio continuum resultsAn area of 7.5 sq deg of the galactic plane at 70 microns have been surveyed with a 1-arcmin beam. The region lies between lII equals 10 deg and lII equals 16 deg and includes the M17 and W33 complexes. The weakest of the 42 sources detected had a flux density of 350 Jy at 70 microns. Detailed far-infrared, (C-12)O, (C-13)O, and radio continuum observations of the sources are presented. The derivation of the important physical parameters of the sources and their surrounding molecular clouds are discussed. The properties of the individual regions are also discussed and maps of selected sources are presented.
Document ID
19820044285
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Stier, M. T. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Fazio, G. G. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Roberge, W. G. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Thum, C. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Wilson, T. L. (Max-Planck-Institut fuer Radioastronomie Bonn, Germany)
Jaffe, D. T. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1982
Publication Information
Publication: Astrophysical Journal Supplement Series
Volume: 48
Subject Category
Astrophysics
Accession Number
82A27820
Funding Number(s)
CONTRACT_GRANT: NGR-22-007-270
Distribution Limits
Public
Copyright
Other

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