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Neutral hydrogen in the Large Magellanic Cloud

Published online by Cambridge University Press:  14 August 2015

R. X. McGee  and
Janice A. Milton
R. X. McGee
Affiliation:
CSIRO Radiophysics Laboratory, Sydney
Janice A. Milton
Affiliation:
CSIRO Radiophysics Laboratory, Sydney

Extract

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The neutral hydrogen gas in the Large Magellanic Cloud has been observed with the 14′.5 beam of the Parkes 210-foot telescope and the 48-channel H-line receiver. We wish to present a progress report based on computer reductions of integrated brightness and median radial velocities for some 4200 profiles. The survey is incomplete for some of the southern regions below dec. −73°. Assisting in the observations were our colleagues, M. W. Sinclair, C. J. Ohlston, and G. H. Trent and the staff at ANRAO, Parkes.

Type
Section II: The Magellanic Clouds
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 289 - 294
Copyright
Copyright © Australian Academy of Science 1964