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Millimeter emission lines in Orion ADuring the course of a search of Orion A for signals from three large organic molecules, several millimeter-wave lines from known interstellar molecules were observed. Results are reported for observations of methanol (CH3OH), methyl cyanide (CH3CN), methyl acetylene (CH3CCH), acetaldehyde (CH3CHO) and (Si-29)O. Emission signals from two hydrogen recombination lines (H41-alpha and H42-alpha) detected from the H II region of Orion A are also reported. Negative results were obtained for several millimeter-wave transitions of ethylene oxide, acetone, and cyclopropenone.
Document ID
19770028828
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lovas, F. J.
(Illinois Univ. Urbana, IL, United States)
Johnson, D. R.
(National Bureau of Standards Washington, D.C., United States)
Buhl, D.
(NASA Goddard Space Flight Center Laboratory for Extraterrestrial Physics, Greenbelt, Md., United States)
Snyder, L. E.
(Illinois, University Urbana, Ill., United States)
Date Acquired
August 8, 2013
Publication Date
November 1, 1976
Publication Information
Publication: Astrophysical Journal
Volume: 209
Subject Category
Astrophysics
Accession Number
77A11680
Distribution Limits
Public
Copyright
Other

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