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Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Convection in 3D Simulations of Red Supergiants
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ALMA detection of CO rotational line emission in red supergiant stars of the massive young star cluster RSGC1
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Signatures of convection in the atmospheres of cool evolved stars
The dusty circumstellar environment of Betelgeuse during the Great Dimming as seen by VLTI/MATISSE
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The Time-averaged Mass-loss Rates of Red Supergiants as Revealed by Their Luminosity Functions in M31 and M33
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Bringing Stellar Evolution and Feedback Together: Summary of Proposals from the Lorentz Center Workshop
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Evolved massive stars at low-metallicity
Ming Yang, Alceste Z. Bonanos, Biwei Jiang, Emmanouil Zapartas, Jian Gao, Yi Ren, Man I. Lam, Tianding Wang, Grigoris Maravelias, Panagiotis Gavras, Shu Wang, Xiaodian Chen, Frank Tramper, Stephan de Wit, Bingqiu Chen, Jing Wen, Jiaming Liu, Hao Tian, Konstantinos Antoniadis and Changqing Luo Astronomy & Astrophysics 676 A84 (2023) https://doi.org/10.1051/0004-6361/202244770
New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars
Early Spectroscopy and Dense Circumstellar Medium Interaction in SN 2023ixf
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