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Notes on the structure of the SMC as observed in 21-cm line radiation from neutral hydrogen

Published online by Cambridge University Press:  14 August 2015

J. V. Hindman
J. V. Hindman*
Affiliation:
CSIRO Radiophysics Laboratory, Sydney

Extract

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Earlier surveys of the line radiation from neutral hydrogen in the Magellanic Clouds (Kerr, Hindman, and Robinson 1954; Hindman, Kerr, and McGee 1963; Hindman et al. 1963) have shown that the amount of gas associated with these extragalactic bodies is relatively large. The gas appears widespread, surrounding the stellar bodies in a single continuous and very tenuous envelope with a marked bridge in the vicinity of the optical wing of the SMC linking the two main concentrations.

Type
Section II: The Magellanic Clouds
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 255 - 261
Copyright
Copyright © Australian Academy of Science 1964 

References

Hindman, J. V., Kerr, F. J., and McGee, R. X. (1963).— Aust. J. Phys. 16: 570–83.Google Scholar
Hindman, J. V., McGee, R. X., Carter, A. W. L., Holmes, E. C. J., and Beard, M. (1963).— Aust. J. Phys. 16: 552–69.Google Scholar
Kerr, F. J., Hindman, J. V., and Robinson, B. J. (1954).— Aust. J. Phys. 7: 297–314.Google Scholar
McGee, R. X., and Murray, J. D. (1963).— Proc. I.R.E. (Aust.) 24: 191–6.Google Scholar