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• W3106155087 abstract "We present results from a study of the eclipsing, colliding-wind binary V444 Cyg that uses a combination of X-ray and optical spectropolarimetric methods to describe the 3-D nature of the shock and wind structure within the system. We have created the most complete X-ray light curve of V444 Cyg to date using 40 ksec of new data from Swift, and 200 ksec of new and archived XMM-Newton observations. In addition, we have characterized the intrinsic, polarimetric phase-dependent behavior of the strongest optical emission lines using data obtained with the University of Wisconsin's Half-Wave Spectropolarimeter. We have detected evidence of the Coriolis distortion of the wind-wind collision in the X-ray regime, which manifests itself through asymmetric behavior around the eclipses in the system's X-ray light curves. The large opening angle of the X-ray emitting region, as well as its location (i.e. the WN wind does not collide with the O star, but rather its wind) are evidence of radiative braking/inhibition occurring within the system. Additionally, the polarimetric results show evidence of the cavity the wind-wind collision region carves out of the Wolf-Rayet star's wind." @default.
• W3106155087 created "2020-11-23" @default.
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• W3106155087 date "2014-12-15" @default.
• W3106155087 modified "2023-10-16" @default.
• W3106155087 title "V444 Cygni X-ray and polarimetric variability: Radiative and Coriolis forces shape the wind collision region" @default.
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• W3106155087 doi "https://doi.org/10.1051/0004-6361/201424468" @default.
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