Modeling the SS 433 Jet Bends

Modeling the SS 433 Jet Bends

We fit Chandra HETGS data obtained for the unusual X-ray binary SS 433. While line strengths and continuum levels hardly change, the jet Doppler shifts show aperiodic variations that probably result from shocks in interactions with the local environment. The X-ray and optical emission line regions a...

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Bibliographic Details
Main Authors: Canizares, Claude R. (Contributor), Schulz, Norbert S. (Contributor), Heinz, Sebastian (Author), Hillwig, Todd C. (Author), Mioduszewski, Amy J. (Author), Marshall, Herman (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor), Marshall, Herman Lee (Contributor)
Format: Article
Language:English
Published: World Scientific, 2012-06-18T13:28:30Z.
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