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A search for interstellar glycineA search has been made for the simplest amino acid - glycine - in Sgr B2, Ori A, and seven other molecular clouds. Six different lines were sought ranging from 83.4 GHz down to 22.7 GHz, and radio telescopes at Parkes, New South Wales, Kitt Peak, Arizona, and Onsala, Sweden, were used. On the assumption of reasonable values for excitation temperature and Boltzmann distributions over rotational energy states, upper limits of column densities for glycine of a few times 10 to the 12th per sq cm to a few times 10 to the 14th per sq cm were typically established in the sources surveyed. Glycine appears to be less abundant than ethanol or ethyl cyanide in molecular clouds such as Sgr B2 and Ori A.
Document ID
19790038740
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Brown, R. D.
(Monash Univ. Clayton, Australia)
Godfrey, P. D.
(Monash Univ. Clayton, Australia)
Storey, J. W. V.
(Monash Univ. Clayton, Australia)
Bassez, M.-P.
(Monash University Clayton, Victoria, Australia)
Robinson, B. J.
(Monash Univ. Clayton, Australia)
Batchelor, R. A.
(Monash Univ. Clayton, Australia)
Mcculloch, M. G.
(Commonwealth Scientific and Industrial Research Organization, Div. of Radiophysics, Epping New South Wales, Australia)
Rydbeck, O. E. H.
(Monash Univ. Clayton, Australia)
Hjalmarson, A. G.
(Onsala Space Observatory Onsala, Sweden)
Date Acquired
August 9, 2013
Publication Date
January 1, 1979
Publication Information
Publication: Royal Astronomical Society
Subject Category
Astrophysics
Accession Number
79A22753
Funding Number(s)
CONTRACT_GRANT: NSF AST-75-20353
CONTRACT_GRANT: NGL-05-003-272
Distribution Limits
Public
Copyright
Other

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