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43. Some problems of meta-galactic radio-emission

Published online by Cambridge University Press:  14 August 2015

I. S. Shklovsky
I. S. Shklovsky*
Affiliation:
Sternberg Astronomical Institute, Moscow, U.S.S.R.

Extract

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The observed cosmical radio-emission has to be divided into the galactic and metagalactic components. The separation of these components is a problem of first importance. It was shown by us (Shklovsky, 1952 [1]) that at least 75% of the observed intensity near the galactic poles is caused by sources located in our stellar system. These sources form an almost spherical sub-system. Another model of the distribution of the cosmical radio-emission sources (Westerhout and Oort, 1951 [2]) is popular in the western countries. The so-called ‘isotropic component’ of metagalactic origin used in that model was considered responsible for the greatest part of the intensity near the galactic poles.

Type
Part III: Galactic Structure and Statistical Studies of Point Sources
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 241 - 243
Copyright
Copyright © Cambridge University Press 1957 

References

1. Shklovsky, I. S. A.J. U.S.S.R. 29, 418, 1952.Google Scholar
2. Westerhout, G. and Oort, J. H. B.A.N. 11, 323, no. 426, 1951.Google Scholar
3. Baldwin, J. Nature , 74, 320, 1954.Google Scholar
4. Shklovsky, I. S. A.J. U.S.S.R. 30, 495, 1953.Google Scholar
5. Shklovsky, I. S. A.J. U.S.S.R. 31, 533, 1954.Google Scholar