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Radio Interferometer Observations of Compact Sources in Supernova Remnants

Published online by Cambridge University Press:  04 August 2017

R. E. Spencer  and
R. Haley
R. E. Spencer
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank Macclesfield, Cheshire, England
R. Haley
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank Macclesfield, Cheshire, England

Extract

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The remains of the progenitor stars of supernovae are likely to have compact radio structure and steep radio spectra, as in the cases of pulsars and SS433. An instrument which is sensitive to compact structure at low frequencies is therefore suitable for a search for new objects. The radio-linked interferometer comprising the MK IA 76m telescope and the Defford 25m telescope situated 127 km to the south has a resolution of ∼1 arcsec at 408 MHz and is ideal for such a task.

Type
V. Compact Objects Associated With Supernova Remnants, Pulsars and Neutron Stars
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 469 - 470
Copyright
Copyright © Reidel 1983 

References

Lyne, A.G., Anderson, B. & Salter, M.J., 1982. Mon. Not. R. astr. Soc., in the press.Google Scholar
Milne, D.K., 1979. Aust. J. Phys., 32, 83.CrossRefGoogle Scholar