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39. The Spatial distribution of radio stars

Published online by Cambridge University Press:  14 August 2015

M. Ryle
M. Ryle*
Affiliation:
Cavendish Laboratory, Cambridge, England

Extract

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The Cambridge survey of radio stars [1], which has been described by Shakeshaft, revealed some 1900 sources of small angular diameter, which appeared to be distributed nearly isotropically. An examination of the number–magnitude distribution shows, however, that they cannot be accounted for in terms of a uniform spatial distribution of sources [2].

Type
Part III: Galactic Structure and Statistical Studies of Point Sources
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 221 - 227
Copyright
Copyright © Cambridge University Press 1957 

References

1. Shakeshaft, J. R., Ryle, M., Baldwin, J. E., Elsmore, B. and Thomson, J. H. Mem. R.A.S. 67, 106, 1955.Google Scholar
2. Ryle, M. and Scheuer, P. A. G. Proc. Roy. Soc. A , 230, 448, 1955.Google Scholar
3. Bondi, H. and Gold, T. M.N.R.A.S. 108, 252, 1948.CrossRefGoogle Scholar
4. Hoyle, F. M.N.R.A.S. 108, 372, 1948.Google Scholar
5. Spitzer, L. and Baade, W. Ap. J. 113, 413, 1951.Google Scholar
6. Palmer, H. P. and Thompson, A. R. This publication, paper 28, p. 162.Google Scholar