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53. On the nature of the emission from the galaxy NGC 4486

Published online by Cambridge University Press:  18 July 2016

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

Extract

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As is known, a striking peculiarity of the radio galaxy NGC 4486 is the presence of a small and very bright ‘jet’ in its central part. As it seems to us, the key to the understanding of the nature of the radio galaxy NGC 4486 is the purely continuous spectrum of the above jet, where not even a slightest trace or emission or absorption lines is present.

Type
Part VII: Additional Contributions
Information
Symposium - International Astronomical Union , Volume 6: Electromagnetic Phenomena in Cosmical Physics , 1958 , pp. 517 - 519
Copyright
Copyright © Cambridge University Press 1958 

References

1. Shklovsky, I. S. A.J. U.S.S.R. 33, no. 3, 1955.Google Scholar