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Evidence for a Radio Brightening Zone Around SS433

Published online by Cambridge University Press:  03 August 2017

R. C. Vermeulen ,
R. T. Schilizzi ,
V. Icke ,
I. Fejes  and
R. E. Spencer
R. C. Vermeulen
Affiliation:
Leiden Observatory, Box 9513, NL-2300 RA, Leiden, NL
R. T. Schilizzi
Affiliation:
NFRA, Box 2, NL-7990 AA, Dwingeloo, NL
V. Icke
Affiliation:
Leiden Observatory, Box 9513, NL-2300 RA, Leiden, NL
I. Fejes
Affiliation:
NFRA, Box 2, NL-7990 AA, Dwingeloo, NL
R. E. Spencer
Affiliation:
NRAL, Jodrell Bank, Macclesfield, Cheshire, SK119 DL, UK

Extract

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SS433 is thought to be a binary system from which two antiparallel beams are ejected at 0.26c. An excellent review of this peculiar object has been given by Margon (1984). The so-called “kinematic model” describes the precessing motion of the beams. They can be obcervef over at least 8 orders of magnitude in distance: from 1012 cm to 1020 cm.

Type
Galactic
Information
Symposium - International Astronomical Union , Volume 129: The Impact of VLBI on Astrophysics and Geophysics , 1988 , pp. 275 - 276
Copyright
Copyright © Reidel 1988 

References

Margon, B. Ann. Rev. Astr. Astrophys. 22, 507–536 (1984)CrossRefGoogle Scholar