{"id":352506,"date":"2026-02-23T19:14:11","date_gmt":"2026-02-23T19:14:11","guid":{"rendered":"https:\/\/www.europesays.com\/ie\/352506\/"},"modified":"2026-02-23T19:14:11","modified_gmt":"2026-02-23T19:14:11","slug":"the-dramatic-transition-of-the-extreme-red-supergiant-woh-g64-to-a-yellow-hypergiant","status":"publish","type":"post","link":"https:\/\/www.europesays.com\/ie\/352506\/","title":{"rendered":"The dramatic transition of the extreme red supergiant WOH\u2009G64 to a yellow hypergiant"},"content":{"rendered":"
  • \n

    Meynet, G. & Maeder, A. Stellar evolution with rotation. X. Wolf\u2013Rayet star populations at solar metallicity. Astron. Astrophys. 404<\/b>, 975\u2013990 (2003).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Ekstr\u00f6m, S. et al. Grids of stellar models with rotation. I. Models from 0.8 to 120 M\u2299 at solar metallicity (Z = 0.014). Astron. Astrophys. 537<\/b>, A146 (2012).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Levesque, E. M. Astrophysics of Red Supergiants 2514\u20133433 (IOP, 2017); https:\/\/doi.org\/10.1088\/978-0-7503-1329-2<\/a><\/p>\n<\/li>\n

  • \n

    Van Dyk, S. D. Red supergiants as supernova progenitors. Galaxies 13<\/b>, 33 (2025).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Li, W. et al. Identification of the red supergiant progenitor of supernova 2005cs: do the progenitors of type II-P supernovae have low mass? Astrophys. J. 641<\/b>, 1060\u20131070 (2006).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Kochanek, C. S. et al. A survey about nothing: monitoring a million supergiants for failed supernovae. Astrophys. J. 684<\/b>, 1336\u20131342 (2008).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Smartt, S. J., Eldridge, J. J., Crockett, R. M. & Maund, J. R. The death of massive stars\u2014I. Observational constraints on the progenitors of type II-P supernovae. Mon. Not. R. Astron. Soc. 395<\/b>, 1409\u20131437 (2009).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Smartt, S. J. Observational constraints on the progenitors of core-collapse supernovae: the case for missing high-mass stars. Publ. Astron. Soc. Aust. 32<\/b>, e016 (2015).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Kochanek, C. S. On the red supergiant problem. Mon. Not. R. Astron. Soc. 493<\/b>, 4945\u20134949 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Fang, Q., Moriya, T. J. & Maeda, K. Red supergiant problem viewed from the nebular phase spectroscopy of type II supernovae. Astrophys. J. 986<\/b>, 39 (2025).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Davies, B. & Beasor, E. R. The \u2018red supergiant problem\u2019: the upper luminosity boundary of type II supernova progenitors. Mon. Not. R. Astron. Soc. 493<\/b>, 468\u2013476 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Davies, B. & Beasor, E. R. \u2019On the red supergiant problem\u2019: a rebuttal, and a consensus on the upper mass cut-off for II-P progenitors. Mon. Not. R. Astron. Soc. 496<\/b>, L142\u2013L146 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Beasor, E. R., Smith, N. & Jencson, J. E. The red supergiant progenitor luminosity problem. Astrophys. J. 979<\/b>, 117 (2025).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Strotjohann, N. L., Ofek, E. O. & Gal-Yam, A. A Bias-corrected luminosity function for red supergiant supernova progenitor stars. Astrophys. J. Lett. 964<\/b>, L27 (2024).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Healy, S., Horiuchi, S. & Ashall, C. The red supergiant problem: as seen from the local group\u2019s red supergiant populations. Preprint at https:\/\/arxiv.org\/abs\/2412.04386<\/a> (2024).<\/p>\n<\/li>\n

  • \n

    De, K. et al. The disappearance of a massive star marking the birth of a black hole in M31. Preprint at https:\/\/arxiv.org\/abs\/2410.14778<\/a> (2024).<\/p>\n<\/li>\n

  • \n

    de Jager, C. The yellow hypergiants. Astron. Astrophys. Rev. 8<\/b>, 145\u2013180 (1998).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Gordon, M. S. & Humphreys, R. M. Red supergiants, yellow hypergiants, and post-RSG evolution. Galaxies 7<\/b>, 92 (2019).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Humphreys, R. M. & Jones, T. J. Episodic gaseous outflows and mass loss from red supergiants. Astron. J. 163<\/b>, 103 (2022).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Jones, T. Red and yellow hypergiants. Galaxies 13<\/b>, 43 (2025).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Humphreys, R. M. The complex upper HR diagram. Galaxies 7<\/b>, 75 (2019).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Meynet, G. et al. Impact of mass-loss on the evolution and pre-supernova properties of red supergiants. Astron. Astrophys. 575<\/b>, A60 (2015).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Zapartas, E. et al. The effect of mass loss in models of red supergiants in the Small Magellanic Cloud. Astron. Astrophys. 697<\/b>, A167 (2025).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Smith, N. Mass loss: its effect on the evolution and fate of high-mass stars. Annu. Rev. Astron. Astrophys. 52<\/b>, 487\u2013528 (2014).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Beasor, E. R. et al. A new mass-loss rate prescription for red supergiants. Mon. Not. R. Astron. Soc. 492<\/b>, 5994\u20136006 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Antoniadis, K. et al. Establishing a mass-loss rate relation for red supergiants in the Large Magellanic Cloud. Astron. Astrophys. 686<\/b>, A88 (2024).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Decin, L., Richards, A. M. S., Marchant, P. & Sana, H. ALMA detection of CO rotational line emission in red supergiant stars of the massive young star cluster RSGC1. Determination of a new mass-loss rate prescription for red supergiants. Astron. Astrophys. 681<\/b>, A17 (2024).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Antoniadis, K. et al. Investigating the metallicity dependence of the mass-loss rate relation of red supergiants. Astron. Astrophys. 702<\/b>, A178 (2025).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Richards, A. M. S., Yates, J. A. & Cohen, R. J. Proper motions of water vapour masers and bipolar outflow from NML Cygni. Mon. Not. R. Astron. Soc. 282<\/b>, 665\u2013676 (1996).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Decin, L. et al. Probing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles. I. Theoretical model\u2014mass-loss history unravelled in VY CMa. Astron. Astrophys. 456<\/b>, 549\u2013563 (2006).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Singh, A. P., Richards, A. M. S., Humphreys, R. M., Decin, L. & Ziurys, L. M. ALMA reveals hidden morphologies in the molecular envelope of VY Canis Majoris. Astrophys. J. Lett. 954<\/b>, L1 (2023).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Glatzel, W. & Kiriakidis, M. Stability of massive stars and the Humphreys\/Davidson limit. Mon. Not. R. Astron. Soc. 263<\/b>, 375 (1993).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Humphreys, R. M. & Davidson, K. Studies of luminous stars in nearby galaxies. III. Comments on the evolution of the most massive stars in the Milky Way and the Large Magellanic Cloud. Astrophys. J. 232<\/b>, 409\u2013420 (1979).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    McDonald, S. L. E., Davies, B. & Beasor, E. R. Red supergiants in M31: the Humphreys\u2013Davidson limit at high metallicity. Mon. Not. R. Astron. Soc. 510<\/b>, 3132\u20133144 (2022).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Schootemeijer, A. et al. A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18. Preprint at https:\/\/arxiv.org\/abs\/2510.12594<\/a> (2025).<\/p>\n<\/li>\n

  • \n

    Landri, C. & Pejcha, O. Driving asymmetric red supergiant winds with binary interactions. Mon. Not. R. Astron. Soc. 531<\/b>, 3391\u20133405 (2024).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    MacLeod, M. et al. Radial velocity and astrometric evidence for a close companion to Betelgeuse. Astrophys. J. 978<\/b>, 50 (2025).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Sana, H. et al. Binary interaction dominates the evolution of massive stars. Science 337<\/b>, 444 (2012).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Ivanova, N. et al. Common envelope evolution: where we stand and how we can move forward. Astron. Astrophys. Rev. 21<\/b>, 59 (2013).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Westerlund, B. E., Olander, N. & Hedin, B. Supergiant and giant M type stars in the Large Magellanic Cloud. Astron. Astrophys. Suppl. 43<\/b>, 267\u2013295 (1981).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Ohnaka, K., Driebe, T., Hofmann, K. H., Weigelt, G. & Wittkowski, M. Spatially resolved dusty torus toward the red supergiant WOH G64 in the Large Magellanic Cloud. Astron. Astrophys. 484<\/b>, 371\u2013379 (2008).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Elias, J. H., Frogel, J. A. & Schwering, P. B. W. Two supergiants in the Large Magellanic Cloud with thick dust shells. Astrophys. J. 302<\/b>, 675 (1986).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Levesque, E. M., Massey, P., Plez, B. & Olsen, K. A. G. The physical properties of the red supergiant WOH G64: the largest star known? Astron. J. 137<\/b>, 4744\u20134752 (2009).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Beasor, E. R. & Smith, N. The extreme scarcity of dust-enshrouded red supergiants: consequences for producing stripped stars via winds. Astrophys. J. 933<\/b>, 41 (2022).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Ohnaka, K. et al. Imaging the innermost circumstellar environment of the red supergiant WOH G64 in the Large Magellanic Cloud. Astron. Astrophys. 691<\/b>, L15 (2024).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    van Loon, J. T., Zijlstra, A. A., Bujarrabal, V. & Nyman, L. \u00c5 Circumstellar masers in the Magellanic Clouds. Astron. Astrophys. 368<\/b>, 950\u2013968 (2001).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Marshall, J. R. et al. Asymptotic giant branch superwind speed at low metallicity. Mon. Not. R. Astron. Soc. 355<\/b>, 1348\u20131360 (2004).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Soszynski, I., Udalski, A., Szymanski, M. K., others, K. & Poleski, R. The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. IV. Long-period variables in the Large Magellanic Cloud. Acta Astron. 59<\/b>, 239\u2013253 (2009).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Boyd, D. Spectroscopic and photometric study of the Mira stars SU Camelopardalis and RY Cephei. J. Am. Assoc. Var. Star Obs. 49<\/b>, 157 (2021).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Kravchenko, K. et al. Tomography of cool giant and supergiant star atmospheres. II. Signature of convection in the atmosphere of the red supergiant star \u03bc Cep. Astron. Astrophys. 632<\/b>, A28 (2019).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Solf, J. Spectral type and luminosity classification of late-type M stars from near-infrared image tube coud\u00e9 spectrograms. Astron. Astrophys. Suppl. Ser. 34<\/b>, 409\u2013416 (1978).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Lamers, H. J. G. L. M., Zickgraf, F.-J., de Winter, D., Houziaux, L. & Zorec, J. An improved classification of B[e]-type stars. Astron. Astrophys. 340<\/b>, 117\u2013128 (1998).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Kraus, M. A census of B[e] supergiants. Galaxies 7<\/b>, 83 (2019).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Rayner, J. T., Cushing, M. C. & Vacca, W. D. The Infrared Telescope Facility (IRTF) spectral library: cool stars. Astrophys. J. Suppl. Ser. 185<\/b>, 289\u2013432 (2009).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Allen, D. A. A catalogue of symbiotic stars. Publ. Astron. Soc. Aust. 5<\/b>, 369\u2013421 (1984).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Miko\u0142ajewska, J. Symbiotic stars: continually embarrassing binaries. Baltic Astron. 16<\/b>, 1\u20139 (2007).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Cowley, A. P. The VV Cephei stars. Publ. Astron. Soc. Pac. 81<\/b>, 297 (1969).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Wright, K. O. The system of VV Cephei derived from an analysis of the H\u03b1 line. J. R. Astron. Soc. Can. 71<\/b>, 152 (1977).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Liimets, T. et al. New insights into the outflows from R Aquarii. Astron. Astrophys. 612<\/b>, A118 (2018).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Soker, N. Close stellar binary systems by grazing envelope evolution. Astrophys. J. 800<\/b>, 114 (2015).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Dori, N., Bear, E. & Soker, N. Wobbling jets in common envelope evolution. Astrophys. J. 954<\/b>, 143 (2023).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Beristain, G., Edwards, S. & Kwan, J. Helium emission from classical T Tauri stars: dual origin in magnetospheric infall and hot wind. Astrophys. J. 551<\/b>, 1037\u20131064 (2001).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Massey, P., Levesque, E. M., Olsen, K. A. G., Plez, B. & Skiff, B. A. HV 11423: the coolest supergiant in the SMC. Astrophys. J. 660<\/b>, 301\u2013310 (2007).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Munoz-Sanchez, G. et al. Episodic mass loss in the very luminous red supergiant [W60] B90 in the Large Magellanic Cloud. Astron. Astrophys. 690<\/b>, A99 (2024).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Dessart, L. & Jacobson-Galan, W. V. A modeling perspective on the diversity of red-supergiant stars exploding within circumstellar material. Preprint at https:\/\/arxiv.org\/abs\/2510.17676<\/a> (2025).<\/p>\n<\/li>\n

  • \n

    Levesque, E. M., Massey, P., Olsen, K. A. G. & Plez, B. Late-type red supergiants: too cool for the Magellanic Clouds? Astrophys. J. 667<\/b>, 202\u2013212 (2007).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Paczy\u0144ski, B. & Sienkiewicz, R. Evolution of close binaries VIII. Mass exchange on the dynamical time scale. Acta Astron. 22<\/b>, 73\u201391 (1972).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Ercolino, A., Jin, H., Langer, N. & Dessart, L. Interacting supernovae from wide massive binary systems. Astron. Astrophys. 685<\/b>, A58 (2024).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Clayton, M., Podsiadlowski, P., Ivanova, N. & Justham, S. Episodic mass ejections from common-envelope objects. Mon. Not. R. Astron. Soc. 470<\/b>, 1788\u20131808 (2017).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Nandez, J. L. A., Ivanova, N. & Lombardi, J. C. J. Recombination energy in double white dwarf formation. Mon. Not. R. Astron. Soc. 450<\/b>, L39\u2013L43 (2015).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Valsan, V., Borges, S. V., Prust, L. & Chang, P. Envelope ejection and the transition to homologous expansion in common-envelope events. Mon. Not. R. Astron. Soc. 526<\/b>, 5365\u20135373 (2023).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Hubble, E. & Sandage, A. The brightest variable stars in extragalactic nebulae. I. M31 and M33. Astrophys. J. 118<\/b>, 353 (1953).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Koumpia, E. et al. Optical and near-infrared observations of the Fried Egg Nebula. Multiple shell ejections on a 100 yr timescale from a massive yellow hypergiant. Astron. Astrophys. 635<\/b>, A183 (2020).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    van Genderen, A. M. et al. Investigation of the pulsations, outbursts, and evolution of the yellow hypergiants: \u03c1 Cas, HR 8752, and HR 5171A, with notes on HD 179821. Astron. Astrophys. 694<\/b>, A136 (2025).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Humphreys, R. M., Jones, T. J. & Gehrz, R. D. The enigmatic object variable A in M33. Astron. J. 94<\/b>, 315 (1987).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Humphreys, R. M. et al. M33\u2019s variable A: a hypergiant star more than 35 years in eruption. Astron. J. 131<\/b>, 2105\u20132113 (2006).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Smith, N. et al. MagAO-X images of the inner core of VY Canis Majoris: a disk and a companion. In American Astronomical Society Meeting Abstracts Vol. 245, 163.13 (American Astronomical Society, 2025).<\/p>\n<\/li>\n

  • \n

    De Beck, E., Andrews, H., Quintana-Lacaci, G. & Vlemmings, W. H. T. The circumstellar environment around the extreme Galactic red supergiant NML Cygni: dense, dusty, and asymmetric. Astron. Astrophys. 698<\/b>, A179 (2025).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Marchant, P. & Bodensteiner, J. The evolution of massive binary stars. Annu. Rev. Astron. Astrophys. 62<\/b>, 21\u201361 (2024).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    van Loon, J. T. & Ohnaka, K. A phoenix rises from the ashes: WOH G64 is still a red supergiant, for now. Preprint at https:\/\/arxiv.org\/abs\/2601.02057<\/a> (2026).<\/p>\n<\/li>\n

  • \n

    Davies, B., Plez, B. & Petrault, M. Explosion imminent: the appearance of red supergiants at the point of core-collapse. Mon. Not. R. Astron. Soc. 517<\/b>, 1483\u20131490 (2022).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Sengupta, S., Sujit, D. & Sarangi, A. Dance to demise\u2014how massive stars may form dense circumstellar shells before explosion. Astrophys. J. 996<\/b>, 18 (2025).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Bronner, V. A., Laplace, E., Schneider, F. R. N. & Podsiadlowski, P. Explosions of pulsating red supergiants: a natural pathway for the diversity of type II-P\/L supernovae. Astron. Astrophys. 703<\/b>, A61 (2025).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Laplace, E., Bronner, V. A., Schneider, F. R. N. & Podsiadlowski, P. Pulsations change the structures of massive stars before they explode: interpreting the nearby supernova SN 2023ixf. Preprint at https:\/\/arxiv.org\/abs\/2508.11088<\/a> (2025).<\/p>\n<\/li>\n

  • \n

    Ercolino, A. et al. The demographics of core-collapse supernovae I. The role of binary evolution and CSM interaction. Preprint at https:\/\/arxiv.org\/abs\/2510.04872<\/a> (2025).<\/p>\n<\/li>\n

  • \n

    Van Dyk, S. D. et al. The progenitor of supernova 1993J revisited. Publ. Astron. Soc. Pac. 114<\/b>, 1322\u20131332 (2002).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Folatelli, G. et al. The progenitor of the type IIb SN 2008ax revisited. Astrophys. J. 811<\/b>, 147 (2015).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    O\u2019Connor, E. & Ott, C. D. Black hole formation in failing core-collapse supernovae. Astrophys. J. 730<\/b>, 70 (2011).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Wright, E. L. et al. The Wide-field Infrared Survey Explorer (WISE): mission description and initial on-orbit performance. Astron. J. 140<\/b>, 1868\u20131881 (2010).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Cutri, R. M. et al. AllWISE data release (Cutri+ 2013). VizieR Online Data Catalog II\/328 https:\/\/ui.adsabs.harvard.edu\/abs\/2014yCat.2328….0C<\/a> (2021).<\/p>\n<\/li>\n

  • \n

    Tonry, J. L. et al. ATLAS: a high-cadence all-sky survey system. Publ. Astron. Soc. Pac. 130<\/b>, 064505 (2018).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Gaia Collaboration et al. The Gaia mission. Astron. Astrophys. 595<\/b>, A1 (2016).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Gaia Collaboration et al. Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674<\/b>, A1 (2023).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Alcock, C. et al. The MACHO Project Large Magellanic Cloud microlensing results from the first two years and the nature of the Galactic dark halo. Astrophys. J. 486<\/b>, 697\u2013726 (1997).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Mainzer, A. et al. Preliminary results from NEOWISE: an enhancement to the Wide-field Infrared Survey Explorer for Solar System science. Astrophys. J. 731<\/b>, 53 (2011).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Udalski, A., Kubiak, M. & Szymanski, M. Optical Gravitational Lensing Experiment. OGLE-2\u2014the second phase of the OGLE project. Acta Astron. 47<\/b>, 319\u2013344 (1997).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Udalski, A. et al. The Optical Gravitational Lensing Experiment. OGLE-III photometric maps of the Large Magellanic Cloud. Acta Astron. 58<\/b>, 89\u2013102 (2008).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Udalski, A., Szyma\u0144ski, M. K. & Szyma\u0144ski, G. OGLE-IV: fourth phase of the Optical Gravitational Lensing Experiment. Acta Astron. 65<\/b>, 1\u201338 (2015).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Heinze, A. N. et al. A first catalog of variable stars measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS). Astron. J. 156<\/b>, 241 (2018).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Shingles, L. et al. Release of the ATLAS Forced Photometry server for public use. Transient Name Server AstroNote 7, 1\u20137 (2021).<\/p>\n<\/li>\n

  • \n

    Alcock, C. et al. Calibration of the MACHO Photometry Database. Publ. Astron. Soc. Pac. 111<\/b>, 1539\u20131558 (1999).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Marshall, J. L. et al. The MagE spectrograph. Proc. SPIE 7014<\/b>, 701454 (2008).<\/p>\n<\/li>\n

  • \n

    Kelson, D. D., Illingworth, G. D., van Dokkum, P. G. & Franx, M. The evolution of early-type galaxies in distant clusters. II. Internal kinematics of 55 galaxies in the z=0.33 cluster CL 1358+62. Astrophys. J. 531<\/b>, 159\u2013183 (2000).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Kelson, D. D. Optimal techniques in two-dimensional spectroscopy: background subtraction for the 21st century. Publ. Astron. Soc. Pac. 115<\/b>, 688\u2013699 (2003).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Dekker, H., D\u2019Odorico, S., Kaufer, A., Delabre, B. & Kotzlowski, H. Iye, M. & Moorwood, A. F. Design, construction, and performance of UVES, the echelle spectrograph for the UT2 Kueyen Telescope at the ESO Paranal Observatory. Proc. SPIE 4008<\/b>, 534\u2013545 (2000).<\/p>\n<\/li>\n

  • \n

    Vernet, J. et al. X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope. Astron. Astrophys. 536<\/b>, A105 (2011).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Ballester, P. et al. The UVES data reduction pipeline. The Messenger 101<\/b>, 31\u201336 (2000).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Modigliani, A. et al. Silva, D. R., Peck, A. B. & Soifer, B. T. Observatory operations: 912 strategies, processes, and systems III. Proc. SPIE 7737<\/b>, 773728 (2010).<\/p>\n<\/li>\n

  • \n

    Smette, A. et al. Molecfit: a general tool for telluric absorption correction. I. Method and application to ESO instruments. Astron. Astrophys. 576<\/b>, A77 (2015).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Houck, J. R. et al. Mather, J. C. (ed.) The infrared spectrograph on the Spitzer Space Telescope Proc. SPIE 5487<\/b>, 62\u201376 (2004).<\/p>\n<\/li>\n

  • \n

    Calzoletti, L. et al. REMIR: the REM infrared camera to follow up the early phases of GRBs afterglows. Nuovo Cimento C 28<\/b>, 759 (2005).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Gustafsson, B. et al. A grid of MARCS model atmospheres for late-type stars. I. Methods and general properties. Astron. Astrophys. 486<\/b>, 951\u2013970 (2008).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    van Loon, J. T., Cioni, M. R. L., Zijlstra, A. A. & Loup, C. An empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich asymptotic giant branch stars. Astron. Astrophys. 438<\/b>, 273\u2013289 (2005).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Jian, M., Matsunaga, N., Jiang, B., Yuan, H. & Zhang, R. Exploring Be phenomena in OBA stars: A mid-infrared search. Astron. Astrophys. 682<\/b>, A59 (2024).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Tabernero, H. M., Dorda, R., Negueruela, I. & Gonz\u00e1lez-Fern\u00e1ndez, C. An LTE effective temperature scale for red supergiants in the Magellanic clouds. Mon. Not. R. Astron. Soc. 476<\/b>, 3106\u20133123 (2018).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Humphreys, R. M., Weis, K., Davidson, K., Bomans, D. J. & Burggraf, B. Luminous and variable stars in M31 and M33. II. Luminous blue variables, candidate LBVs, Fe II emission line stars, and other supergiants. Astrophys. J. 790<\/b>, 48 (2014).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Bergemann, M., Kudritzki, R.-P., Gazak, Z., Davies, B. & Plez, B. Red supergiant stars as cosmic abundance probes. III. NLTE effects in J-band magnesium lines. Astrophys. J. 804<\/b>, 113 (2015).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Accetta, K. et al. The Seventeenth Data Release of the Sloan Digital Sky Surveys: complete release of MaNGA, MaStar, and APOGEE-2 data. Astrophys. J. Suppl. Ser. 259<\/b>, 35 (2022).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    de Wit, S. et al. Properties of luminous red supergiant stars in the Magellanic Clouds. Astron. Astrophys. 669<\/b>, A86 (2023).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Patrick, L. R. et al. Red supergiant stars in binary systems. I. Identification and characterization in the small magellanic cloud from the UVIT ultraviolet imaging survey. Mon. Not. R. Astron. Soc. 513<\/b>, 5847\u20135860 (2022).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Neugent, K. F., Massey, P., Skiff, B. & Meynet, G. Yellow and red supergiants in the Large Magellanic Cloud. Astrophys. J. 749<\/b>, 177 (2012).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Mathewson, D. S. & Clarke, J. N. Supernova remnants in the Large Magellanic Cloud. Astrophys. J. 180<\/b>, 725\u2013738 (1973).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    van Loon, J. T., Hekkert, P. T. L., Bujarrabal, V., Zijlstra, A. A. & Nyman, L.-A. Discovery of H2O maser emission from the red supergiant IRAS04553\u22126825 in the Large Magellanic Cloud. Astron. Astrophys. 337<\/b>, 141\u2013144 (1998).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Kravchenko, K. et al. Atmosphere of Betelgeuse before and during the Great Dimming event revealed by tomography. Astron. Astrophys. 650<\/b>, L17 (2021).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Kourniotis, M., Kraus, M., Maryeva, O., Borges Fernandes, M. & Maravelias, G. Revisiting the evolved hypergiants in the Magellanic Clouds. Mon. Not. R. Astron. Soc. 511<\/b>, 4360\u20134376 (2022).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Humphreys, R. M., Jones, T. J. & Martin, J. C. Yellow supergiants and post-red supergiant evolution in the Large Magellanic Cloud. Astron. J. 166<\/b>, 50 (2023).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Lobel, A. et al. High-resolution spectroscopy of the yellow hypergiant \u03c1 Cassiopeiae from 1993 through the outburst of 2000\u20132001. Astrophys. J. 583<\/b>, 923\u2013954 (2003).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    van Genderen, A. M. et al. Pulsations, eruptions, and evolution of four yellow hypergiants. Astron. Astrophys. 631<\/b>, A48 (2019).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Nieuwenhuijzen, H. et al. The hypergiant HR 8752 evolving through the yellow evolutionary void. Astron. Astrophys. 546<\/b>, A105 (2012).<\/p>\n

    Article<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Oudmaijer, R. D., Groenewegen, M. A. T., Matthews, H. E., Blommaert, J. A. D. L. & Sahu, K. C. The spectral energy distribution and mass-loss history of IRC+10420. Mon. Not. R. Astron. Soc. 280<\/b>, 1062\u20131070 (1996).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Nieuwenhuijzen, H. & de Jager, C. Checking the yellow evolutionary void. Three evolutionary critical hypergiants: HD 33579, HR 8752 & IRC +10420. Astron. Astrophys. 353<\/b>, 163\u2013176 (2000).<\/p>\n

    ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Dotter, A. MESA Isochrones and Stellar Tracks (MIST) 0: Methods for the construction of stellar isochrones. Astrophys. J. Suppl. Ser. 222<\/b>, 8 (2016).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Choi, J. et al. Mesa Isochrones and Stellar Tracks (MIST). I. Solar-scaled models. Astrophys. J. 823<\/b>, 102 (2016).<\/p>\n

    Article<\/a>\u00a0
    \n     ADS<\/a>\u00a0
    \n
    \n Google Scholar<\/a>\u00a0\n <\/p>\n<\/li>\n

  • \n

    Munoz-Sanchez, G. et al. The dramatic transition of the extreme red supergiant WOH G64 to a yellow hypergiant. figshare https:\/\/doi.org\/10.6084\/m9.figshare.30738671<\/a> (2025).<\/p>\n<\/li>\n","protected":false},"excerpt":{"rendered":"Meynet, G. & Maeder, A. Stellar evolution with rotation. X. Wolf\u2013Rayet star populations at solar metallicity. Astron. Astrophys.…\n","protected":false},"author":2,"featured_media":352507,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":"","_share_on_mastodon":"0"},"categories":[77],"tags":[582,1778,18,910,19,17,452,133,1240,31765],"class_list":["post-352506","post","type-post","status-publish","format-standard","has-post-thumbnail","category-science","tag-astronomy","tag-astrophysics-and-cosmology","tag-eire","tag-general","tag-ie","tag-ireland","tag-physics","tag-science","tag-stars","tag-stellar-evolution"],"share_on_mastodon":{"url":"https:\/\/pubeurope.com\/@ie\/116121549188469105","error":""},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts\/352506","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/comments?post=352506"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts\/352506\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/media\/352507"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/media?parent=352506"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/categories?post=352506"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/tags?post=352506"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}