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POSYDON Version 2: Population Synthesis with Detailed Binary-evolution Simulations across a Cosmological Range of Metallicities
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Development of convective envelopes in massive stars
A trifecta of modelling tools: a Bayesian binary black hole model selection combining population synthesis and galaxy formation models
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Gaia BH1 and BH2 – evolutionary models with overshooting of the black hole progenitors within the present-day binary separation
Evolved Massive Stars at Low Metallicity. VII. The Lower Mass Limit of the Red Supergiant Population in the Large Magellanic Cloud
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Evolution of rotating massive stars adopting a newer, self-consistent wind prescription at Small Magellanic Cloud metallicity
The boring history of Gaia BH3 from isolated binary evolution
Giuliano Iorio, Stefano Torniamenti, Michela Mapelli, Marco Dall’Amico, Alessandro A. Trani, Sara Rastello, Cecilia Sgalletta, Stefano Rinaldi, Guglielmo Costa, Bera A. Dahl-Lahtinen, Gastón J. Escobar, Erika Korb, M. Paola Vaccaro, Elena Lacchin, Benedetta Mestichelli, Ugo N. Di Carlo, Mario Spera and Manuel Arca Sedda Astronomy & Astrophysics 690 A144 (2024) https://doi.org/10.1051/0004-6361/202450531
Giant Eruptions in Massive Stars and their Effect on the Stellar Structure
Modelling stellar evolution in mass-transferring binaries and gravitational-wave progenitors with metisse
Poojan Agrawal, Jarrod Hurley, Simon Stevenson, Carl L Rodriguez, Dorottya Szécsi and Alex Kemp Monthly Notices of the Royal Astronomical Society 525(1) 933 (2023) https://doi.org/10.1093/mnras/stad2334
Three Dimensional Natures of Massive Star Envelopes