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Shock-heated radiation-driven outflows as a solution to the weak-wind problem of late O-type stars

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Why binary interaction does not necessarily dominate the formation of Wolf-Rayet stars at low metallicity

T. Shenar, A. Gilkis, J. S. Vink, H. Sana and A. A. C. Sander
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Evolution of rotation in rapidly rotating early-type stars during the main sequence with 2D models

D. Gagnier, M. Rieutord, C. Charbonnel, B. Putigny and F. Espinosa Lara
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New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars

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Self-consistent Solutions for Line-driven Winds of Hot Massive Stars: The m-CAK Procedure

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PoWR grids of non-LTE model atmospheres for OB-type stars of various metallicities

R. Hainich, V. Ramachandran, T. Shenar, et al.
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The shortest-period Wolf-Rayet binary in the Small Magellanic Cloud: Part of a high-order multiple system

T. Shenar, R. Hainich, H. Todt, et al.
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Helium Star Models with Optically Thick Winds: Implications for the Internal Structures and Mass-loss Rates of Wolf–Rayet Stars

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