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Detection of the torsionally excited state of methanol in Orion ATorsionally excited methanol has been detected in Orion A, where three emission lines observed in the region of 93-100 GHz coincide with laboratory measurements of three methanol transitions. Torsionally excited methanol may therefore be used as a novel temperature probe, since this state lies near 200 per cm above the ground state, or about 290 K. No emission was detected from the transition arising from levels near 300 per cm, or approximately 430 K above the ground state.
Document ID
19820041531
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lovas, F. J.
(National Bureau of Standards Washington, DC, United States)
Suenram, R. D.
(National Bureau of Standards Washington, DC, United States)
Snyder, L. E.
(Illinois, University Urbana, IL, United States)
Hollis, J. M.
(NASA Goddard Space Flight Center Laboratory for Astronomy and Solar Physics, Greenbelt, MD, United States)
Lees, R. M.
(New Brunswick, University Fredericton, Canada)
Date Acquired
August 10, 2013
Publication Date
February 1, 1982
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
82A25066
Funding Number(s)
CONTRACT_GRANT: NSF AST-79-07830
Distribution Limits
Public
Copyright
Other

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