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Cited article:

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Modeling the Optical to Ultraviolet Polarimetric Variability from Thomson Scattering in Colliding-wind Binaries

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The Wolf–Rayet + Black Hole Binary NGC 300 X-1: What is the Mass of the Black Hole?

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V444 Cygni X-ray and polarimetric variability: Radiative and Coriolis forces shape the wind collision region

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A 2007 photometric study and UV spectral analysis of the Wolf‐Rayet binary V444 Cyg

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X-ray emission characteristics of two Wolf-Rayet binaries: V444 Cyg and CD Cru

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Monthly Notices of the Royal Astronomical Society 402 (3) 1767 (2010)

Wolf‐Rayet Mass‐Loss Limits Due to Frequency Redistribution

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Lower mass loss rates in O-type stars: Spectral signatures of dense clumps in the wind of two Galactic O4 stars

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