Abstract
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.
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Fürst, E., Reich, W., Beck, R., Hirth, W., Angerhofer, P.: 1982, Astron. Astrophys., in press
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© 1983 IAU
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Fürst, E., Reich, W., Hirth, W. (1983). Radio Observations of Small Diameter Sources in the Direction of Old Supernova Remnants. In: Danziger, J., Gorenstein, P. (eds) Supernova Remnants and their X-Ray Emission. International Astronomical Union / Union Astronomique Internationale, vol 101. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7231-5_41
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DOI: https://doi.org/10.1007/978-94-009-7231-5_41
Publisher Name: Springer, Dordrecht
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