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The IACOB project
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X-Shooting ULLYSES: Massive stars at low metallicity
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Stripped Helium Star and Compact Object Binaries in Coeval Populations: Predictions Based on Detailed Binary Evolution Models
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Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
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F Rizzuti, R Hirschi, V Varma, W D Arnett, C Georgy, C Meakin, M Mocák, A StJ Murphy and T Rauscher Monthly Notices of the Royal Astronomical Society 533(1) 687 (2024) https://doi.org/10.1093/mnras/stae1778
3D simulations of a neon burning convective shell in a massive star
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Data mining techniques on astronomical spectra data – III. Association analysis
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Modelling Time-dependent Convective Penetration in 1D Stellar Evolution
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F Rizzuti, R Hirschi, W D Arnett, C Georgy, C Meakin, A StJ Murphy, T Rauscher and V Varma Monthly Notices of the Royal Astronomical Society 523(2) 2317 (2023) https://doi.org/10.1093/mnras/stad1572
Modelling stellar evolution in mass-transferring binaries and gravitational-wave progenitors with metisse
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Bringing Stellar Evolution and Feedback Together: Summary of Proposals from the Lorentz Center Workshop
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3D hydrodynamic simulations of massive main-sequence stars – I. Dynamics and mixing of convection and internal gravity waves
Falk Herwig, Paul R Woodward, Huaqing Mao, William R Thompson, Pavel Denissenkov, Josh Lau, Simon Blouin, Robert Andrassy and Adam Paul Monthly Notices of the Royal Astronomical Society 525(2) 1601 (2023) https://doi.org/10.1093/mnras/stad2157
Core overshoot constrained by the absence of a solar convective core and some solar-like stars
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The spins of stripped B stars support magnetic internal angular momentum transport
Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars
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Convective core entrainment in 1D main-sequence stellar models
Superadiabaticity and the metallicity independence of the Humphreys–Davidson limit
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The role of mass transfer and common envelope evolution in the formation of merging binary black holes
Grids of stellar models with rotation – V. Models from 1.7 to 120 M⊙ at zero metallicity
Laura J Murphy, Jose H Groh, Sylvia Ekström, et al. Monthly Notices of the Royal Astronomical Society 501(2) 2745 (2021) https://doi.org/10.1093/mnras/staa3803
The R136 star cluster dissected with Hubble Space Telescope/STIS – II. Physical properties of the most massive stars in R136
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The effects of surface fossil magnetic fields on massive star evolution – II. Implementation of magnetic braking in mesa and implications for the evolution of surface rotation in OB stars
Z Keszthelyi, G Meynet, M E Shultz, et al. Monthly Notices of the Royal Astronomical Society 493(1) 518 (2020) https://doi.org/10.1093/mnras/staa237
Type IIP Supernova Progenitors. III. Blue to Red Supergiant Ratio in Low-metallicity Models with Convective Overshoot
Relative importance of convective uncertainties in massive stars
Etienne A Kaiser, Raphael Hirschi, W David Arnett, et al. Monthly Notices of the Royal Astronomical Society 496(2) 1967 (2020) https://doi.org/10.1093/mnras/staa1595
snapshot: connections between internal and surface properties of massive stars
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Massive donors in interacting binaries: effect of metallicity
High-resolution Observations of Cen A: Yellow and Red Supergiants in a Region of Jet-induced Star Formation?*
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