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SiS in Orion-KL - Evidence for 'outflow' chemistryThe J = 6-5 and J = 5-4 rotational transitions at 91 and 109 GHz toward Orion-KL provide evidence for the presence of SiS at an LSR velocity of 7.5 km/sec and with a half-width at zero power of 36 km/sec. The estimated current density corresponds to a fractal abundance of about 4 x 10 to the -9th. The implied SiO/SiS ratio of about 60 is close to the cosmic O/S ratio of about 40 and is much less than that predicted by ion-molecule models. Other unidentified lines near 91 and 109 have been identified.
Document ID
19880036613
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ziurys, L. M.
(Five College Radio Astronomy Observatory Amherst, MA, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1988
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 324
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
88A23840
Funding Number(s)
CONTRACT_GRANT: NSF AST-82-12252
CONTRACT_GRANT: NAGW-436
Distribution Limits
Public
Copyright
Other

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