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Cited article:

The geometry and dynamical role of stellar wind bubbles in photoionized H ii regions

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Monthly Notices of the Royal Astronomical Society 501 (1) 1352 (2020)
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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)
https://doi.org/10.1051/0004-6361/201833419

Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant High Mass X-Ray Binaries

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Space Science Reviews 212 (1-2) 59 (2017)
https://doi.org/10.1007/s11214-017-0340-1

Macroclumping as solution of the discrepancy between Hαand P v mass loss diagnostics for O-type stars

B. Šurlan, W.-R. Hamann, A. Aret, et al.
Astronomy & Astrophysics 559 A130 (2013)
https://doi.org/10.1051/0004-6361/201322390

Predictions for mass-loss rates and terminal wind velocities of massive O-type stars

L. E. Muijres, Jorick S. Vink, A. de Koter, P. E. Müller and N. Langer
Astronomy & Astrophysics 537 A37 (2012)
https://doi.org/10.1051/0004-6361/201015818

NLTE models of line-driven stellar winds - III. Influence of X-ray radiation on wind structure of O stars

Jiří Krtička and Jiří Kubát
Monthly Notices of the Royal Astronomical Society 394 (4) 2065 (2009)
https://doi.org/10.1111/j.1365-2966.2009.14457.x