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Radio-Emission from Supernovae Remnants in Distant Galaxies

Published online by Cambridge University Press:  14 August 2015

P. Notni ,
H. Oleak  and
G.-M. Richter
P. Notni
Affiliation:
Zentralinstitut für Astrophysik, Potsdam, G.D.R.
H. Oleak
Affiliation:
Zentralinstitut für Astrophysik, Potsdam, G.D.R.
G.-M. Richter
Affiliation:
Zentralinstitut für Astrophysik, Potsdam, G.D.R.

Abstract

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It is suggested that some 5C2 radio sources previously identified with normal spiral galaxies, are associated with supernova remnants in these galaxies. This hypothesis is tested by the relative radio and optical positions and by luminosity estimates. It could be further tested by possible coincidences of Ohio radio sources with known supernovae, and also by predicted decreases in radio emission.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 44: External Galaxies and Quasi-Stellar Objects , 1972 , pp. 82 - 86
Copyright
Copyright © Reidel 1972 

References

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