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Atmospheric NLTE models for the spectroscopic analysis of blue stars with winds
Free accessIV. Porosity in physical and velocity spaceEDP Sciences | 2018| -
2D wind clumping in hot, massive stars from hydrodynamical line-driven instability simulations using a pseudo-planar approach
Free accessEDP Sciences | 2018| -
Wind Roche lobe overflow in high-mass X-ray binaries
Free accessA possible mass-transfer mechanism for ultraluminous X-ray sourcesEDP Sciences | 2019| -
New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars
II. A grid of O-type stars in the Galaxy and the Magellanic CloudsEDP Sciences | 2021| -
Line-driven ablation of circumstellar discs - I. Optically thin decretion discs of classical Oe/Be stars
Oxford University Press | 2016| -
Mass loss from inhomogeneous hot star winds
Free accessIII. An effective-opacity formalism for line radiative transfer in accelerating, clumped two-component media, and first results on theory and diagnosticsEDP Sciences | 2014| -
Mass loss from inhomogeneous hot star winds
Free accessI. Resonance line formation in 2D modelsEDP Sciences | 2010| -
Mass loss from inhomogeneous hot star winds I. Resonance line formation in 2D models
Free accessArXiv | 2009|
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