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Radiation-driven winds of hot luminous stars

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Determination of physical parameters of particle-accelerating colliding-wind binaries based on generalized partition considerations

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New Challenges for Wind Shock Models: TheChandraSpectrum of the Hot Star δ Orionis

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XMM‐NewtonDetection of Hard X‐Ray Emission in the Nitrogen‐Type Wolf‐Rayet Star WR 110

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XMM‐Newtonand Very Large Array Observations of the Variable Wolf‐Rayet Star EZ Canis Majoris: Evidence for a Close Companion?

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Non-spherical evolution of the line-driven wind instability

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X‐Ray Modeling of Very Young Early‐Type Stars in the Orion Trapezium: Signatures of Magnetically Confined Plasmas and Evolutionary Implications

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Constraints fromInfrared Space ObservatoryData on the Velocity Law and Clumpiness of WR 136

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An Intrinsic Absorption Complex toward RX J1230.8+0115: Geometry and Photoionization Conditions

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Wind inhibition by X-ray irradiation in HMXBs: the influence of clumping and the final X-ray luminosity

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A mass-loss rate determination for ζ Puppis from the quantitative analysis of X-ray emission-line profiles

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Moving inhomogeneous envelopes of stars

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Cosmic Gamma-Ray Sources

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Chandra grating spectroscopy of embedded wind shock X-ray emission from O stars shows low plasma temperatures and significant wind absorption

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Light variations due to the line-driven wind instability and wind blanketing in O stars

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Investigation of the WR 11 field at decimeter wavelengths

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Long-term soft and hard X-ray investigation of the colliding wind WN+O binary WR 25

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