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...
Main Authors: | Laurent, Philippe (Author), Bel, Marion Cadolle (Author), Pottschmidt, Katja (Author), Pooley, Guy (Author), Bodaghee, Arash (Author), Rodriguez, Jerome (Author), Grinberg, Victoria (Contributor), Wilms, Jorn (Author), Gouiffes, Christian (Author) |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research (Contributor) |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2015-09-03T18:23:54Z.
|
Subjects: | |
Online Access: | Get fulltext |
Similar Items
-
CHANDRA X-RAY SPECTROSCOPY OF THE FOCUSED WIND IN THE CYGNUS X-1 SYSTEM. I. THE NONDIP SPECTRUM IN THE LOW/HARD STATE
by: Hanke, Manfred, et al.
Published: (2015) -
Spectroscopy of the Stellar Wind in the Cygnus X-1 System
by: I. Miškovičová, et al.
Published: (2011-01-01) -
The behavioural ecology of the whooper swan (Cygnus cygnus cygnus)
by: Brazil, Mark Andrew
Published: (1981) -
CORONA, JET, AND RELATIVISTIC LINE MODELS FOR SUZAKU/RXTE/CHANDRA-HETG OBSERVATIONS OF THE CYGNUS X-1 HARD STATE
by: Nowak, Michael A., et al.
Published: (2015) -
Cygnus
by: Totovic, Bojana
Published: (2016)