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Neutral Hydrogen Observations of NGC 5236

Published online by Cambridge University Press:  25 April 2016

B.M. Lewis
B.M. Lewis*
Affiliation:
Mount Stromlo Observatory, Australian National University, Canberra
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Extract

NGC 5236 is the fourth galaxy beyond the local group to be investigated at Parkes. Most of the observations were made with a single-channel 21 cm line receiver, coupled to the 210 ft dish. The half-power beamwidth is 13´.5. Declination scans were made through the galaxy, and treated by methods already established for NGC 551, NGC 3002 and NGC 31093. The peak antenna temperature is 1.5°K.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 3 , February 1968 , pp. 104 - 105
Copyright
Copyright © Astronomical Society of Australia 1968

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References

1 Robinson, B.J. and van Damme, K.J., Aust. J. Phys., 19, 111 (1966).Google Scholar
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3 van Damme, K.J., Aust. J. Phys., 19, 687 (1966).Google Scholar
4 Roberts, M.S., Preprint, National Radio Observatory, Greenbank (1966).Google Scholar
5 Danver, C.G., Ann. Lund. Obs., No. 10 (1942).Google Scholar
6 van Damme, K.J., personal communication.Google Scholar
7 de Vaucouleurs, G., and Page, Judith, Ap. J., 136, 107 (1962).Google Scholar