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Models of molecular clouds and the abundances of H2CO and HCO/+/Observations of HCO(+) and H2CO in a sample of 13 molecular clouds have been analyzed by construction of uniform, spherical cloud models. The total densities and the abundance of HCO(+) and H2CO relative to H2 which result from these models fall into two domains: one group of clouds has a low temperature, moderate density, and high abundances; the other group has higher temperature and density, but lower abundances. The factor distinguishing these groups may be depletion onto grains in the denser sources.
Document ID
19810028412
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Wootten, A.
(Texas, University Austin, Tex.; Owens Valley Radio Observatory, Pasadena, Calif., United States)
Snell, R.
(Texas Univ. Austin, TX, United States)
Evans, N. J., II
(Texas, University Austin, Tex., United States)
Date Acquired
August 11, 2013
Publication Date
September 1, 1980
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
81A12816
Funding Number(s)
CONTRACT_GRANT: NSF AST-77-00247
CONTRACT_GRANT: NSF AST-77-28475
CONTRACT_GRANT: NSG-7381
Distribution Limits
Public
Copyright
Other

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