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Cited article:

Boron depletion in Galactic early B-type stars reveals two different main sequence star populations

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Rotational mixing in Be stars: nitrogen abundances for a sample of Be stars from the MiMeS survey

A. Ahmed and T. A. A. Sigut
Monthly Notices of the Royal Astronomical Society 471 (3) 3398 (2017)
https://doi.org/10.1093/mnras/stx1737

Spitzerinfrared spectrograph point source classification in the Small Magellanic Cloud

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Monthly Notices of the Royal Astronomical Society 451 (4) 3504 (2015)
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EVOLUTION OF MASS FUNCTIONS OF COEVAL STARS THROUGH WIND-MASS LOSS AND BINARY INTERACTIONS

F. R. N. Schneider, R. G. Izzard, N. Langer and S. E. de Mink
The Astrophysical Journal 805 (1) 20 (2015)
https://doi.org/10.1088/0004-637X/805/1/20

Magnetic main sequence stars as progenitors of blue supergiants

I. Petermann, N. Castro and N. Langer
Proceedings of the International Astronomical Union 9 (S307) 391 (2014)
https://doi.org/10.1017/S1743921314007224

THE ROTATION RATES OF MASSIVE STARS: THE ROLE OF BINARY INTERACTION THROUGH TIDES, MASS TRANSFER, AND MERGERS

S. E. de Mink, N. Langer, R. G. Izzard, H. Sana and A. de Koter
The Astrophysical Journal 764 (2) 166 (2013)
https://doi.org/10.1088/0004-637X/764/2/166

Probing the models: Abundances for high-mass stars in binaries

K. Pavlovski, J. Southworth, K. Pavlovski, A. Tkachenko and G. Torres
EAS Publications Series 64 29 (2013)
https://doi.org/10.1051/eas/1364004