Abstract
We review the X-ray and millimeter observations of the W50 lobes associated with the twin-jet source SS 433. This study is aimed at shedding light on the energetics from SS 433, understanding the asymmetries of the lobes, and testing for cosmic ray acceleration in a Galactic twin-jet source.
NSERC fellow
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Dubner, G., et al: 1998, Astron. Astrophys. 116, 1842.
Durouchoux, P., et al: 1998, in: Proc. of the 32nd COSPAR meeting, Nagoya, Japan.
Kotani, T.: 1997, Ph.D. thesis, University of Tokyo, ISAS, RN 655.
Safi-Harb, S. and Ögelman, H.: 1997, Astrophys. J. 483, 868.
Safl-Harb, S. and Petre, R.: 1999, Astrophys. J. 512, 784.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2001 Springer Science+Business Media New York
About this paper
Cite this paper
Safi-Harb, S., Durouchoux, P., Petre, R. (2001). The Galactic Microquasar W50 / SS 433 System. In: Castro-Tirado, A.J., Greiner, J., Paredes, J.M. (eds) Microquasars. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0700-9_36
Download citation
DOI: https://doi.org/10.1007/978-94-010-0700-9_36
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3828-7
Online ISBN: 978-94-010-0700-9
eBook Packages: Springer Book Archive