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Numerical Simulations of the Precessing Jets of SS433

Published online by Cambridge University Press:  25 May 2016

E. Müller  and
W. Brinkmann
E. Müller
Affiliation:
MPI für Astrophysik, Karl-Schwarzschild-Strasse 1, 85740 Garching, Germany
W. Brinkmann
Affiliation:
MPI für Astrophysik, Karl-Schwarzschild-Strasse 1, 85740 Garching, Germany

Abstract

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The unique Galactic object SS433 contains the best-studied relativistic jets, and their physical parameters (velocity, temperature, density) are known to an astronomically unprecedented accuracy, i.e., to factors of order unity. The comparison of numerical simulations of these jets with observations provides deeper insight into the SS433/W50 system and is ideal for testing our understanding of the jet phenomenon in general.

Type
Part II: Posters
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 415 - 416
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Brinkmann, W., Aschenbach, B., & Kawai, N. 1996, A&A, 312, 306.Google Scholar
Brinkmann, W., Kawai, N., Matsuoka, M., & Fink, H. H. 1991, A&A, 241, 112.Google Scholar
Margon, B. 1984, ARA&A, 22, 507.Google Scholar
Müller, E., & Brinkmann, W. 2000, A&A, submitted.Google Scholar
Yamauchi, S., Kawai, N., & Aoki, T. 1994, PASJ, 46, L109.Google Scholar