Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-13T04:30:39.906Z Has data issue: false hasContentIssue false
  • English
  • Français

Large HI clouds in the Galaxy

Published online by Cambridge University Press:  14 August 2015

R. X. McGee
R. X. McGee*
Affiliation:
CSIRO Radiophysics Laboratory, Sydney

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

van de Hulst (1958), in giving representative sizes of the structural details of the interstellar medium, lists the dimensions of a typical cloud, seen in 21-cm emission, as 20–70 pc but warns that we should not be surprised to find different “sizes of interstellar clouds” determined from different sets of data.

Type
Section 1: The Galaxy
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 126 - 130
Copyright
Copyright © Australian Academy of Science 1964 

References

van de Hulst, H. C. (1958).— Rev. Mod. Phys. 30: 913–23. Symp. IAU 8: 913–23. [Cambridge, Mass. 1957.] Google Scholar
Kerr, F. J. (1962).— M.N. 123: 327–45.Google Scholar
Kerr, F. J., Hindman, J. V., and Carpenter, Martha Stahr (1957).— Nature 180: 677–9.Google Scholar
McGee, R. X., and Murray, J. D. (1961).— Aust. J. Phys. 14: 260–78.Google Scholar
McGee, R. X., and Murray, J. D. (1963).— Proc. I.R.E. (Aust.) 24: 191–6.Google Scholar
McGee, R. X., Murray, J. D., and Milton, Janice A. (1963).— Aust. J. Phys. 16: 136–70.Google Scholar