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Supernova Remnants with Radio Jets

Published online by Cambridge University Press:  04 August 2017

M.J. Kesteven ,
J.L. Caswell ,
R.S. Roger ,
D.K. Milne ,
R.F. Haynes  and
K.J. Wellington
M.J. Kesteven
Affiliation:
Division of Radiophysics, CSIRO, PO Box 76, Epping, NSW 2121 Australia
J.L. Caswell
Affiliation:
Division of Radiophysics, CSIRO, PO Box 76, Epping, NSW 2121 Australia
R.S. Roger
Affiliation:
Division of Radiophysics, CSIRO, PO Box 76, Epping, NSW 2121 Australia
D.K. Milne
Affiliation:
Division of Radiophysics, CSIRO, PO Box 76, Epping, NSW 2121 Australia
R.F. Haynes
Affiliation:
Division of Radiophysics, CSIRO, PO Box 76, Epping, NSW 2121 Australia
K.J. Wellington
Affiliation:
Division of Radiophysics, CSIRO, PO Box 76, Epping, NSW 2121 Australia

Extract

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Two examples are given of probable radio jet/supernova remnant association, G332.4+0.1 and G315.8-0.0. In both cases the jet length is larger than the radius of the remnant's shell; the jet diameter is barely resolved, and is substantially less than the observed shell thickness. The jet luminosity is 5–10% that of the shell. The G332.4+0.1 jet termi nates in an extended plume whose luminosity is ∼50% that of the shell.

Type
I. Rotation-Powered Pulsars
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 125
Copyright
Copyright © Reidel 1987