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Convective-core overshooting and the final fate of massive stars
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Grids of Wolf–Rayet Stars Using MESA with the k − ω Model: From 25 to 120 M
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Melnick 33Na: a very massive colliding-wind binary system in 30 Doradus
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Cygnus X-1 contains a 21–solar mass black hole—Implications for massive star winds
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Ionizing photon production of Population III stars: effects of rotation, convection, and initial mass function
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Relative importance of convective uncertainties in massive stars
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Theoretical investigation of the Humphreys–Davidson limit at high and low metallicity
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Convective H–He interactions in massive population III stellar evolution models