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Molecular gas temperature and density in spiral galaxiesWe combine beam-matched CO-13, CO-12 J = 3 yields 2 and J = 2 yields 1 line data to infer the molecular gas excitation conditions in the central 500 to 1600 pc diameters of a small sample of infrared-bright external galaxies: NGC253, IC342, M 83, Maffei 2, and NGC6946. Additional observations of the J = 1 yields 0 lines of C-18O and CO-13 set limits on the opacity of the CO-13 J = 1 yields 0 line averaged over the central kiloparsec of these spiral galaxies.
Document ID
19930017603
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Wall, W. F.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Jaffe, D. T.
(Texas Univ. Austin., United States)
Bash, F. N.
(Texas Univ. Austin., United States)
Israel, F. P.
(Leiden Univ. Netherlands)
Maloney, P. R.
(NASA Ames Research Center Moffett Field, CA., United States)
Baas, F.
(Joint Astronomy Centre Hilo, HI., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1993
Publication Information
Publication: NASA. Ames Research Center, The Evolution of Galaxies and Their Environment
Subject Category
Astrophysics
Accession Number
93N26792
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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