Polarized Gamma-ray Emission from the Galactic Black Hole Cygnus X-1

Details Polarized Gamma-ray Emission from the Galactic Black Hole Cygnus X-1 Polarized Gamma-ray Emission from the Galactic Black Hole Cygnus X-1

2011-04-21

arxiv.org/abs/1104.4282v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

11 pages, 3 figures, to be published in Science in April 22nd 2011, available on Science Express Web site (March 24th edition)

Scientific paper

Because of their inherently high flux allowing the detection of clear signals, black hole X-ray binaries are interesting candidates for polarization studies, even if no polarization signals have been observed from them before. Such measurements would provide further detailed insight into these sources' emission mechanisms. We measured the polarization of the gamma-ray emission from the black hole binary system Cygnus X-1 with the INTEGRAL/IBIS telescope. Spectral modeling of the data reveals two emission mechanisms: The 250-400 keV data are consistent with emission dominated by Compton scattering on thermal electrons and are weakly polarized. The second spectral component seen in the 400keV-2MeV band is by contrast strongly polarized, revealing that the MeV emission is probably related to the jet first detected in the radio band.

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