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Cited article:

The impact of initial mass dependent convective boundary mixing on the structure and fates of massive stars

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Pulsations Change the Structures of Massive Stars before Explosion: Interpreting SN 2023ixf and SN 2024ggi

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Validating a non-local stellar convection model with 3D hydrodynamics simulations

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It’s written in the massive stars: The role of stellar physics in the formation of black holes

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Explodability criteria for the neutrino-driven supernova mechanism

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Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. III. The Mass-loss and Evolutionary Pathways of the Red Supergiant Progenitors

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A Late-time View of the Progenitor Candidates of the Type II-P SN 2009ib and SN 2012ec

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Explosions of pulsating red supergiants: A natural pathway for the diversity of Type II-P/L supernovae

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SN 2017ckj: A linearly declining type IIb supernova with a relatively massive hydrogen envelope

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Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star

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Gaia BH1 and BH2 – evolutionary models with overshooting of the black hole progenitors within the present-day binary separation

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Merger seismology: Distinguishing massive merger products from genuine single stars using asteroseismology

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