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Chandra spectral measurements of the O supergiant ζ Puppis indicate a surprising increase in the wind mass-loss rate over 18 yr

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The chaotic wind of WR 40 as probed by BRITE

Tahina Ramiaramanantsoa, Richard Ignace, Anthony F J Moffat, et al.
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3D MHD simulations and synthetic radio emission from an oblique rotating magnetic massive star

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Theoretical wind clumping predictions of OB supergiants from line-driven instability simulations across the bi-stability jump

F. A. Driessen, J. O. Sundqvist and N. D. Kee
Astronomy & Astrophysics 631 A172 (2019)
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Coordinated UV and X-Ray Spectroscopic Observations of the O-type Giant ξ Per: The Connection between X-Rays and Large-scale Wind Structure* †

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New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars

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Bondi–Hoyle–Lyttleton accretion in supergiant X-ray binaries: stability and disc formation

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Clumpy wind accretion in Supergiant X-ray Binaries

Ileyk El Mellah, Andreas A. C. Sander, Jon O. Sundqvist and Rony Keppens
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Wind inhibition by X-ray irradiation in HMXBs: the influence of clumping and the final X-ray luminosity

J. Krtička, J. Kubát and I. Krtičková
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