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The Secondary Component of the Extremely Low Mass Ratio Massive Binary HD 165246 Revealed by GHOST
C. N. Rodriguez, T. Ansin, G. A. Ferrero, O. G. Benvenuto, R. Gamen, N. I. Morrell, J. I. Arias, R. E. Higa, C. Putkuri, C. Johnston, K. Chiboucas, E. Deibert, C. R. Hayes, J.-E. Heo, M. Jeong, V. Kalari, E. Martioli, V. M. Placco, K. A. Venn, S. Xu, R. Diaz, M. Gomez-Jimenez, R. Ruiz-Carmona, C. Simpson, A. W. McConnachie, et al. The Astrophysical Journal 980(2) 169 (2025) https://doi.org/10.3847/1538-4357/ada892
The Potential of Asteroseismology to Resolve the Blue Supergiant Problem
Earl Patrick Bellinger, Selma E. de Mink, Walter E. van Rossem and Stephen Justham The Astrophysical Journal Letters 967(2) L39 (2024) https://doi.org/10.3847/2041-8213/ad4990
Observational mapping of the mass discrepancy in eclipsing binaries: Selection of the sample and its photometric and spectroscopic properties
Andrew Tkachenko, Krešimir Pavlovski, Nadezhda Serebriakova, Dominic M. Bowman, Luc IJspeert, Sarah Gebruers and John Southworth Astronomy & Astrophysics 683 A252 (2024) https://doi.org/10.1051/0004-6361/202347793
Asteroseismic modelling of fast rotators and its opportunities for astrophysics
X-Shooting ULLYSES: Massive stars at low metallicity
M. Bernini-Peron, A. A. C. Sander, V. Ramachandran, L. M. Oskinova, J. S. Vink, O. Verhamme, F. Najarro, J. Josiek, S. A. Brands, P. A. Crowther, V. M. A. Gómez-González, A. C. Gormaz-Matamala, C. Hawcroft, R. Kuiper, L. Mahy, W. L. F. Marcolino, L. P. Martins, A. Mehner, T. N. Parsons, D. Pauli, T. Shenar, A. Schootemeijer, H. Todt and J. Th. van Loon Astronomy & Astrophysics 692 A89 (2024) https://doi.org/10.1051/0004-6361/202450475
Merger seismology: Distinguishing massive merger products from genuine single stars using asteroseismology
Numerical experiments to help understand cause and effect in massive star evolution
Eoin Farrell, Jose H Groh, Georges Meynet and J J Eldridge Monthly Notices of the Royal Astronomical Society 512(3) 4116 (2022) https://doi.org/10.1093/mnras/stac538
The spins of stripped B stars support magnetic internal angular momentum transport
Grids of stellar models with rotation VII: models from 0.8 to 300 M⊙ at supersolar metallicity (Z = 0.020)
Norhasliza Yusof, Raphael Hirschi, Patrick Eggenberger, et al. Monthly Notices of the Royal Astronomical Society 511(2) 2814 (2022) https://doi.org/10.1093/mnras/stac230
One size does not fit all: Evidence for a range of mixing efficiencies in stellar evolution calculations