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Far-infrared, submillimeter, and millimeter spectroscopy of the Galactic center - Radio ARC and +20/+50 kilometer per second cloudsResults are presented from FIR, sub-mm, and mm spectroscopic observations of the radio arc and the +20/+50 km/s molecular clouds in the Galactic center. The results for the radio arc are analyzed, including the spatial distribution of C II forbidden line emission, the spatial distribution of CO emission, the luminosity and mass of C(+) regions, and the CO 7 - 6 emission and line profiles. Model calculations are used to study molecular gas in the radio arc. In addition, forbidden C II, CO 7 - 6, and C(O-18) mapping is presented for the +20/+50 km/x clouds. Consideration is given to the impact of the results on the interpretation of the physical conditions, excitation, and heating of the gas clouds in the arc and near the center.
Document ID
19900049589
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Genzel, R.
(Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Harris, A. I.
(Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Geis, N.
(Max-Planck-Institut fuer extraterrestrische Physik Garching, Federal Republic of Germany, United States)
Stacey, G. J.
(Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Townes, C. H.
(California, University Berkeley, United States)
Date Acquired
August 14, 2013
Publication Date
June 10, 1990
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 356
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
90A36644
Funding Number(s)
CONTRACT_GRANT: NAG2-208
Distribution Limits
Public
Copyright
Other

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