Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-25T03:00:39.504Z Has data issue: false hasContentIssue false

The radio emission from the galaxy and the andromeda nebula

Published online by Cambridge University Press:  27 June 2016

J. E. Baldwin*
Affiliation:
Cavendish Laboratory, Cambridge, England

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.

Although the sources responsible for the radio emission from the Galaxy are unknown, it may nevertheless be valuable to make a comparison between the magnitude and distribution of the emission observed in our Galaxy and that of other nebulae. Analyses have already been made to relate the total emitted power from nearby nebulae with that from the Galaxy, and by considering the integrated radiation from well-defined clusters attempts were made to extend the comparison to the average emission from fainter nebulae.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1958 

References

REFERENCES

1. Hanbury Brown, R. and Hazard, C. Phil. Mag. 43, 137, 1952.Google Scholar
2. Baldwin, J. E. and Elsmore, B. Nature, 173, 818, 1954.Google Scholar
3. Baade, W. and Minkowski, R. Ap. J. 119, 215, 1954.CrossRefGoogle Scholar
4. Westerhout, G. and Oort, J. H. B.A.N. 11, 323, 1951.Google Scholar
5. Shklovsky, I. S. Ast. Zh. 29, 418, 1952.Google Scholar
6. Ryle, M. and Hewish, A. Mem. R.A.S. 67, 97, 1955.Google Scholar
7. Baldwin, J. E. Nature, 174, 320, 1954.Google Scholar
8. Baade, W. Reported in Sky and Telescope, 14, 371, 1955.Google Scholar