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Radio Observations of Small Diameter Sources in the Direction of Old Supernova Remnants

Published online by Cambridge University Press:  04 August 2017

E. Fürst ,
W. Reich  and
W. Hirth
E. Fürst
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, FRG
W. Reich
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, FRG
W. Hirth
Affiliation:
Astronomisches Institut der Universität, Bonn, FRG

Extract

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Radio observations with high sensitivity have shown that lots of more or less compact structures can be found in the field of extended and old supernova remnants (SNRs). These small diameter sources have been subject to many recent observations. The aim of these studies is to infer a possible physical association of these sources with the SNR shell. The interest in this link is based on various aspects, instabilities of shocked interstellar matter, star formation, etc.

Type
II. Middle Aged and Older Supernova Remnants
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 287 - 288
Copyright
Copyright © Reidel 1983 

References

Fürst, E., Reich, W., Beck, R., Hirth, W., Angerhofer, P.: 1982, Astron. Astrophys., in press Google Scholar