V444 Cygni X-ray and polarimetric variability: radiative and coriolis forces shape the wind collision region

Autor: Lomax, JR, Nazé, Y, Hoffman, JL, Russell, CMP, De Becker, M, Corcoran, MF, Davidson, JW, Neilson, HR, Owocki, S, Pittard, JM, Pollock, AMT
Jazyk: angličtina
Rok vydání: 2015
Předmět:
ISSN: 0004-6361
Popis: 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 3D 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 ks of new data from Swift, and 200 ks 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.
Databáze: OpenAIRE