Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-27T04:47:35.031Z Has data issue: false hasContentIssue false

High-Resolution Maps of Two Supernova Remnants

Published online by Cambridge University Press:  25 April 2016

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

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
Copyright
Copyright © Astronomical Society of Australia 1983

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Caswell, J.L., Haynes, R.F., Milne, D.K., and Wellington, K.J., Mon. Not. R. Astron. Soc, 203, 595 (1983).Google Scholar
Caswell, J.L., and Lerche, I., Mon. Not. R. Astron. Soc, 187, 201 (1983).Google Scholar
Clark, D.H., Caswell, J.L., and Green, A.J., Aust. J. Phys. Astrophys. Suppl. No. 37, 1 (1975).Google Scholar
Clark, D.H., and Caswell, J.L., Mon. Not. R. Astron. Soc, 174, 267 (1976).Google Scholar
Mills, B.Y., Proc Astron. Soc. Aust., 4, 156 (1981).Google Scholar
Milne, D.K., Goss, W.M., Haynes, R.F., Wellington, K.J., Caswell, J.L., and Skellern, D.J., Mon. Not. R. Astron. Sor., 188, 437 (1979).Google Scholar
Milne, D.K., Proc. Astron. Soc. Aust., 3, 341 (1979).CrossRefGoogle Scholar