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Cited article:

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A Deep Exposure in High Resolution X-Rays Reveals the Hottest Plasma in the ζ Puppis Wind

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

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Measuring the stellar wind parameters in IGR J17544-2619 and Vela X-1 constrains the accretion physics in supergiant fast X-ray transient and classical supergiant X-ray binaries

A. Giménez-García, T. Shenar, J. M. Torrejón, et al.
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Influence of X-ray radiation on the hot star wind ionization state and on the radiative force

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Advances in Space Research 58 (5) 710 (2016)
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A COORDINATED X-RAY AND OPTICAL CAMPAIGN OF THE NEAREST MASSIVE ECLIPSING BINARY,δORIONIS Aa. IV. A MULTIWAVELENGTH, NON-LTE SPECTROSCOPIC ANALYSIS

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Influence of extreme ultraviolet radiation on the P vionization fraction in hot star winds

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X-ray emission from hydrodynamical wind simulations in non-LTE models

Jiri Krtička, Achim Feldmeier, Lidia M. Oskinova, Jiri Kubát and Wolf-Rainer Hamann
Proceedings of the International Astronomical Union 6 (S272) 614 (2010)
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