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Interstellar hydrogen sulfide.Hydrogen sulfide has been detected in seven Galactic sources by observation of a single line corresponding to the rotational transition from the 1(sub 10) to the 1(sub 01) levels at 168.7 GHz. The observations show that hydrogen sulfide is only a moderately common interstellar molecule comparable in abundance to H2CO and CS, but somewhat less abundant than HCN and much less abundant than CO.
Document ID
19720057605
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Thaddeus, P.
Kutner, M. L.
(NASA Goddard Institute for Space Studies New York, N.Y., United States)
Penzias, A. A.
Wilson, R. W.
Jefferts, K. B.
(Bell Telephone Laboratories, Inc. Murray Hill, N.J., United States)
Date Acquired
August 6, 2013
Publication Date
September 1, 1972
Publication Information
Publication: Astrophysical Journal
Volume: 176
Subject Category
Space Sciences
Accession Number
72A41271
Distribution Limits
Public
Copyright
Other

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