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Interaction of the SS433 Jet with the Interstellar Medium

Published online by Cambridge University Press:  25 May 2016

P. O'Neill ,
R. Sood ,
P. Durouchoux  and
S. Safi-Harb
P. O'Neill
Affiliation:
School of Physics, University College, University of New South Wales, Australian Defence Force Academy, Canberra, ACT 2600, Australia
R. Sood
Affiliation:
School of Physics, University College, University of New South Wales, Australian Defence Force Academy, Canberra, ACT 2600, Australia
P. Durouchoux
Affiliation:
CE Saclay, DSM, DAPNIA, Service d'Astrophysique, Cedex, France
S. Safi-Harb
Affiliation:
NASA, GSFC, Code 662, Greenbelt, MD 20771, U.S.A.

Abstract

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X-ray emission observed from the SS433/W50 system has been interpreted as resulting from the interaction of the binary jets with the surrounding medium. We have been carrying out millimetre wavelength measurements of this system. We find no evidence for the association of a molecular cloud with the eastern jet, but we do find evidence for a strong association with the western jet.

Type
Part II: Posters
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 419 - 420
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Durouchoux, P., et al. 2000, Adv. Space Res., in press.Google Scholar
Margon, B. 1984, ARA&A, 22, 507.Google Scholar
Safi-Harb, S., & Ogelman, H. 1997, ApJ, 483, 868.Google Scholar