Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-30T16:38:48.849Z Has data issue: false hasContentIssue false
  • English
  • Français

Part III: General Summarizing Discussion of Problems Raised in Parts I and II

Published online by Cambridge University Press:  03 August 2017

Abstract

An abstract is not available for this content so a preview has been provided. As you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Discussion
Information
Symposium - International Astronomical Union , Volume 8: Cosmical Gas Dynamics , July 1958 , pp. 994 - 1008
Copyright
Copyright © American Physical Society 1958 

References

1 van de Hulst, H. C. and Burgers, J. M., editors, I. A. U. Symposium No. 2 (North-Holland Publishing Company, Amsterdam, The Netherlands, 1955).Google Scholar

2 See reference 1, p. 154.Google Scholar

3 See reference 1, p. 145.Google Scholar

4 See reference 1, pp. 127–129.Google Scholar

5 Hall, J. S. and Mikesell, A. H., Publ. U. S. Nav. Observ. 17, Part I (1950).Google Scholar

6 Hiltner, W. A., Astrophys. J. 114, 241 (1954).Google Scholar

7 Hiltner, W. A., Astrophys. J. Suppl. II, No. 24, 389 (1956).Google Scholar

∗ Note added by editor in proof .—Dieter's thesis, Harvard, 1958, presents evidence for a halo in M 33. Peak emission —4°K; velocity dispersion —50 km/sec; density ∼0.1 M H within radius 34 kpc; total halo mass ∼3% mass M 33.Google Scholar

8 Biermann, L., Kosmische Physik , edited by Heisenberg, W. (Springer-Verlag, Berlin, 1953), second edition, Chap. I. 4.Google Scholar