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Title:
Supernova remnants with jets
Authors:
Kesteven, M. J.; Caswell, J. L.; Milne, D. K.; Haynes, R. F.; Roger, R. S.
Affiliation:
AA(CSIRO, Div. of Radiophysics, Epping, Australia), AB(CSIRO, Div. of Radiophysics, Epping, Australia), AC(CSIRO, Div. of Radiophysics, Epping, Australia), AD(CSIRO, Div. of Radiophysics, Epping, Australia), AE(Dominion Radiophysical Observatory, Penticton, Australia)
Publication:
(Joint USSR-Australia Shklovskii Memorial Symposium on Supernova Remnants and Pulsars, Pushchino, USSR, June 8-11, 1986) Australian Journal of Physics (ISSN 0004-9506), vol. 40, no. 6, 1987, p. 855-859.
Publication Date:
00/1987
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
RADIO JETS (ASTRONOMY), SUPERNOVA REMNANTS, CRAB NEBULA, LUMINOSITY
Bibliographic Code:
1987AuJPh..40..855K

Abstract

Two examples are given of probable radio jet/supernova remnant associations: 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, and the jet diameter is barely resolved and substantially less than the observed shell thickness. The jet luminosity is 5-10 percent that of the shell. The G332.4 + 0.1 jet terminates in an extended plume whose luminosity is about 50 percent that of the shell.

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