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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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Line-drag damping of Alfvén waves in radiatively driven winds of magnetic massive stars

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X-ray spectroscopy of the γ-ray brightest nova V906 Car (ASASSN-18fv)

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

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

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

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3D MHD simulations and synthetic radio emission from an oblique rotating magnetic massive star

S Daley-Yates, I R Stevens and A ud-Doula
Monthly Notices of the Royal Astronomical Society 489 (3) 3251 (2019)
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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
Astronomy & Astrophysics 620 A150 (2018)
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Non-axisymmetric line-driven disc winds II - full velocity gradient

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Clumpy wind accretion in Supergiant X-ray Binaries

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Subphotospheric fluctuations in magnetized radiative envelopes: contribution from unstable magnetosonic waves

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