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Exploring the connection between atmosphere models and evolution models of very massive stars
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X-Shooting ULLYSES: Massive stars at low metallicity
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Development of convective envelopes in massive stars
Empirical mass-loss rates and clumping properties of O-type stars in the Large Magellanic Cloud
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X-Shooting ULLYSES: Massive stars at low metallicity
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Evidence for very massive stars in extremely UV-bright star-forming galaxies at z ∼ 2.2–3.6
A. Upadhyaya, R. Marques-Chaves, D. Schaerer, F. Martins, I. Pérez-Fournon, A. Palacios and E. R. Stanway Astronomy & Astrophysics 686 A185 (2024) https://doi.org/10.1051/0004-6361/202449184
Two waves of massive stars running away from the young cluster R136
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X-Shooting ULLYSES: Massive stars at low metallicity
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Carbon monoxide cooling in radiative transfer modelling of supernovae
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The rates and host galaxies of pair-instability supernovae through cosmic time: predictions from BPASS and IllustrisTNG
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Analysis of FUV Emission in the Vicinity of R136 Cluster in 30 Doradus
Barenya Kumar Dev, Gautam Saikia, Olag Pratim Bordoloi, P. Shalima and Rupjyoti Gogoi Journal of Physics: Conference Series 2919(1) 012013 (2024) https://doi.org/10.1088/1742-6596/2919/1/012013
Very massive stars and pair-instability supernovae: mass-loss framework for low metallicity
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Constraints on the multiplicity of the most massive stars known: R136 a1, a2, a3, and c
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An observed population of intermediate-mass helium stars that have been stripped in binaries
M. R. Drout, Y. Götberg, B. A. Ludwig, J. H. Groh, S. E. de Mink, A. J. G. O’Grady and N. Smith Science 382(6676) 1287 (2023) https://doi.org/10.1126/science.ade4970
Mass-loss implementation and temperature evolution of very massive stars
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Melnick 33Na: a very massive colliding-wind binary system in 30 Doradus
Joachim M Bestenlehner, Paul A Crowther, Patrick S Broos, Andrew M T Pollock and Leisa K Townsley Monthly Notices of the Royal Astronomical Society 510(4) 6133 (2022) https://doi.org/10.1093/mnras/stab3521
A systematic study of super-Eddington layers in the envelopes of massive stars
The Uncertain Future of Massive Binaries Obscures the Origin of LIGO/Virgo Sources
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X-ray properties of early-type stars in the Tarantula Nebula from T-ReX
Paul A Crowther, Patrick S Broos, Leisa K Townsley, Andy M T Pollock, Katie A Tehrani and Marc Gagné Monthly Notices of the Royal Astronomical Society 515(3) 4130 (2022) https://doi.org/10.1093/mnras/stac1952
Spectroscopic evolution of very massive stars at Z = 1/2.5 Z⊙
Explaining the differences in massive star models from various simulations
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Very massive star winds as sources of the short-lived radioactive isotope 26Al
The hydrogen clock to infer the upper stellar mass
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High-contrast and resolution near-infrared photometry of the core of R136
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Formation of GW190521 from stellar evolution: the impact of the hydrogen-rich envelope, dredge-up, and 12C(α, γ)16O rate on the pair-instability black hole mass gap
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Superadiabaticity and the metallicity independence of the Humphreys–Davidson limit
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Massive Black Holes Regulated by Luminous Blue Variable Mass Loss and Magnetic Fields
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VLT/X-shooter spectroscopy of massive young stellar objects in the 30 Doradus region of the Large Magellanic Cloud
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The expansion of stripped-envelope stars: Consequences for supernovae and gravitational-wave progenitors
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Effects of winds on the leftover hydrogen in massive stars following Roche lobe overflow
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Massive Stars in the Tarantula Nebula: A Rosetta Stone for Extragalactic Supergiant HII Regions
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The impact of stars stripped in binaries on the integrated spectra of stellar populations
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Very massive stars: a metallicity-dependent upper-mass limit, slow winds, and the self-enrichment of globular clusters
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