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Hydrogen sulfide in a circumstellar envelopeA search for hydrogen sulfide in the cool circumstellar envelopes of 25 stars was made using the 1(10)-1(01) rotational line at 1.8 mm. It was detected in the bipolar nebula/OH maser OH231.8+4.2, an object having a high rate of mass loss. An approximate analysis indicates that 1/60 of the sulfur in this outflowing envelope is in the form of H2S, a fraction which may be similar to that in the atmosphere of the central star. In addition, the shape of the observed line profile is discussed in terms of a possible variation of the outflow velocity with latitude above the system's equatorial plane.
Document ID
19830050516
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ukita, N.
(Institut de Radio Astronomie Millimetrique Saint-Martin-d'Heres, Isere, France)
Morris, M.
(Columbia University New York, NY; California, University, Los Angeles, CA, United States)
Date Acquired
August 11, 2013
Publication Date
May 1, 1983
Publication Information
Publication: Astronomy and Astrophysics
Volume: 121
Issue: 1, Ma
ISSN: 0004-6361
Subject Category
Astrophysics
Accession Number
83A31734
Distribution Limits
Public
Copyright
Other

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