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The Corona Australis Dark Cloud

Published online by Cambridge University Press:  25 April 2016

R. A. Vaile  and
K. N. R. Taylor
R. A. Vaile
Affiliation:
Astrophysics Group, School of Physics, University of N.S.W.
K. N. R. Taylor
Affiliation:
Astrophysics Group, School of Physics, University of N.S.W.
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Extract

The Corona Australis cometary globule is a large southern object known to be a region of slow star formation. We have mapped the complex in the 21cm hydrogen line and preliminary results are reported in Llewellyn et al. (1981) and Taylor et al. (1981). The most extensive A, map of the region is given by Rossano (1978) and is based on star counts.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 4 , 1982 , pp. 443 - 447
Copyright
Copyright © Astronomical Society of Australia 1982

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References

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