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Hydrogen-line observations of the galactic centre region

Published online by Cambridge University Press:  14 August 2015

F. J. Kerr
F. J. Kerr*
Affiliation:
CSIRO Radiophysics Laboratory, Sydney

Extract

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A detailed study of the galactic centre region is being made with the 210-foot telescope at Parkes and a 48-channel hydrogen-line receiver. Line profiles have been recorded on a 6-min-of-arc grid over a central area 2° square, and also along the galactic equator and a number of other longitude lines. These observations, which have been partially reduced, show that the structure and motions of the gas are very complex in the neighbourhood of the centre.

Type
Section 1: The Galaxy
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 187 - 191
Copyright
Copyright © Australian Academy of Science 1964 

References

Drake, F. D. (1959).—NRAO Ann. Rep. No. 1: 2.Google Scholar
Rougoor, G. W., and Oort, J. H. (1960).— Proc. Nat. Acad. Sci. (Washington) 46: 1–13.CrossRefGoogle Scholar