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Identification of interstellar methanol linesThe extended internal axis method Hamiltonian of Herbst et al. (1984) was used to study the rotational spectrum of methanol out to high values of the rotational quantum number J. Laboratory data for 783 lines of (C-12)H3OH from the lowest three torsional levels out to a rotational quantum number of J = 22 were fitted to an rms deviation of 4.40 MHz. For (C-13)H3OH, 455 lines out to J = 22 were fitted to an rms of 2.28 MHz.
Document ID
19890023063
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Sutton, E. C.
(California, University Berkeley, United States)
Herbst, Eric
(Duke University Durham, NC, United States)
Date Acquired
August 13, 2013
Publication Date
October 1, 1988
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 333
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
89A10434
Funding Number(s)
CONTRACT_GRANT: NAGW-189
CONTRACT_GRANT: NSF AST-87-15295
Distribution Limits
Public
Copyright
Other

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