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36. On the nature of the emission from the Galaxy NGC4486

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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It is well known that the radio galaxy NGC4486 has as a striking peculiarity a small and very bright ‘jet’ in its central part. It seems to us that the key to the understanding of the nature of this radio galaxy is the purely continuous spectrum of the jet, where not even a slight trace of emission or absorption lines is present.

Type
Part II: Point Sources: Individual Study and Physical Theory
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 205 - 207
Copyright
Copyright © Cambridge University Press 1957 

References

1. Shklovsky, I. S. Proc. Acad. Sci. U.S.S.R. 90, 983, 1953.Google Scholar
2. Shklovsky, I. S. Astr. Zj. 33, N 3, 1955.Google Scholar
3. Baade, W. Ap. J. 123, 550, 1956.Google Scholar