POLARIMETRY AND THE HIGH-ENERGY EMISSION MECHANISMS IN QUASAR JETS: THE CASE OF PKS 1136-135

Since the discovery of kiloparsec-scale X-ray emission from quasar jets, the physical processes responsible for their high-energy emission have been poorly defined. A number of mechanisms are under active debate, including synchrotron radiation, inverse-Comptonized cosmic microwave background (IC/CM...

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Bibliographic Details
Main Authors: Cara, Mihai (Author), Perlman, Eric S. (Author), Uchiyama, Yasunobu (Author), Cheung, Chi C. (Author), Coppi, Paolo (Author), Georganopoulos, Markos (Author), Worrall, Diana M. (Author), Stawarz, Lukasz (Author), Begelman, Mitchell C. (Author), O'Dea, Christopher P. (Author), Baum, Stefi A. (Author), Marshall, Herman (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor), Marshall, Herman Lee (Contributor)
Format: Article
Language:English
Published: Institute of Physics/American Astronomical Society, 2015-02-12T18:30:11Z.
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