SPECTRAL STATE DEPENDENCE OF THE 0.4–2 MEV POLARIZED EMISSION IN CYGNUS X-1 SEEN WITH INTEGRAL/IBIS, AND LINKS WITH THE AMI RADIO DATA

Polarization of the [> over ~] 400 keV hard tail of the microquasar Cygnus X-1 has been independently reported by INTEGRAL/Imager on Board the INTEGRAL Satellite (IBIS), and INTEGRAL/SPectrometer on INTEGRAL and interpreted as emission from a compact jet. These conclusions were, however, based on...

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Bibliographic Details
Main Authors: Laurent, Philippe, Bel, Marion Cadolle, Pottschmidt, Katja, Pooley, Guy, Bodaghee, Arash, Rodriguez, Jerome, Grinberg, Victoria, Wilms, Jorn, Gouiffes, Christian
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: IOP Publishing 2015
Online Access:http://hdl.handle.net/1721.1/98363
https://orcid.org/0000-0003-2538-0188