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Ammonia in the Hot Galactic Centre Cloud G 1.6-0.025

Published online by Cambridge University Press:  25 April 2016

F. F. Gardner ,
J. B. Whiteoak ,
J. R. Forster ,
W. L. Peters  and
T. B. H. Kuiper
F. F. Gardner
Affiliation:
Division of Radiophysics, CSIRO, Sydney
J. B. Whiteoak
Affiliation:
Division of Radiophysics, CSIRO, Sydney
J. R. Forster
Affiliation:
Division of Radiophysics, CSIRO, Sydney
W. L. Peters
Affiliation:
Mount Stromlo and Siding Spring Observatories, ANU
T. B. H. Kuiper
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California
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Abstract

As 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 G1.6-0.025. 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.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 6 , Issue 2 , 1985 , pp. 176 - 180
Copyright
Copyright © Astronomical Society of Australia 1985

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References

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