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Cited article:

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Wind properties of Milky Way and SMC massive stars: empirical Z dependence from cmfgen models

W L F Marcolino, J -C Bouret, H J Rocha-Pinto, M Bernini-Peron and J S Vink
Monthly Notices of the Royal Astronomical Society 511 (4) 5104 (2022)
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The SOFIA FEEDBACK Legacy Survey Dynamics and Mass Ejection in the Bipolar H ii Region RCW 36

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New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars

J. O. Sundqvist, R. Björklund, J. Puls and F. Najarro
Astronomy & Astrophysics 632 A126 (2019)
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Demonstration of a Novel Method for Measuring Mass-loss Rates for Massive Stars

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The pulsating magnetosphere of the extremely slowly rotating magnetic β Cep star ξ1 CMa

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No breakdown of the radiatively driven wind theory in low-metallicity environments★†

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DIVISION G COMMISSION 36: THEORY OF STELLAR ATMOSPHERES

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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)
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X‐ray emission from massive stars with magnetic fields

L.M. Oskinova, W.‐R. Hamann, J.P. Cassinelli, J.C. Brown and H. Todt
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