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Far-infrared Spectroscopy of Galaxies: the 158 Micron C(+) LineThe C II 158 micron fine structure line in six gas rich galaxies was investigated. These data are combined with other measurements of the C II line (in various galactic sources) and are compared to studies of the CO J = approaches O rotational line at 2.6 mm, the H I 21 cm line, and the far infrared continuum emission in the same objects.
Document ID
19850009573
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Crawford, M. K. (California Univ. Berkeley, CA, United States)
Genzel, R. L. (California Univ. Berkeley, CA, United States)
Townes, C. H. (California Univ. Berkeley, CA, United States)
Watson, D. M. (California Inst. of Tech.)
Date Acquired
August 12, 2013
Publication Date
December 1, 1984
Publication Information
Publication: NASA. Ames Research Center Airborne Astron. Symp.
Subject Category
Astronomy
Accession Number
85N17882
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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