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Ammonia in the hot galactic centre cloud G 1.6-0.025As part of an extensive southern survey of interstellar NH3 with the Parkes 64-m radio telescope (with a beamwidth of 81 arcsec), the (1,1), (2,2), and (3,3) transitions have been observed towards the galactic centre molecular cloud Gl.6-0.025. The cloud has an overall size of 10 arcmin, and contains several concentrations with differing velocities. It has several features also observed in other galactic centre clouds, e.g. high optical depths and kinetic temperatures above 50 K.
Document ID
19860053851
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Gardner, F. F.
(Commonwealth Scientific and Industrial Research Organization Sydney, Australia)
Whiteoak, J. B.
(Commonwealth Scientific and Industrial Research Organization Sydney, Australia)
Forster, J. R.
(CSIRO Div. of Radiophysics, Sydney, Australia)
Peters, W. L.
(Mount Stromlo and Siding Spring Observatories Canberra, Australia)
Kuiper, T. B. H.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1985
Publication Information
Publication: Astronomical Society of Australia, Proceedings
Volume: 6
Issue: 2, 19
ISSN: 0066-9997
Subject Category
Astrophysics
Accession Number
86A38589
Distribution Limits
Public
Copyright
Other

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