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High-Resolution Maps of Two Supernova Remnants

Published online by Cambridge University Press:  25 April 2016

J.L. Caswell ,
R.F. Haynes ,
D.K. Milne ,
K.J. Wellington  and
R.M. Smith
J.L. Caswell
Affiliation:
Division of Radiophysics, CSIRO, Sydney
R.F. Haynes
Affiliation:
Division of Radiophysics, CSIRO, Sydney
D.K. Milne
Affiliation:
Division of Radiophysics, CSIRO, Sydney
K.J. Wellington
Affiliation:
Division of Radiophysics, CSIRO, Sydney
R.M. Smith
Affiliation:
Mount Stromlo and Siding Spring Observatories, ANU
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Extract

High-resolution radio maps of supernova remnants (SNRs) are indispensable for distinguishing the more common shell remnants from the centrally concentrated (Crab-like) remnants; such studies also reveal any departures from symmetry, and this can yield vital information concerning interaction of the ejecta with the surrounding interstellar medium.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 2 , 1983 , pp. 227 - 229
Copyright
Copyright © Astronomical Society of Australia 1983

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References

Caswell, J.L., Haynes, R.F., Milne, D.K., and Wellington, K.J., Mon. Not. R. Astron. Soc, 203, 595 (1983).Google Scholar
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