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This article has been cited by the following article(s):
The Time-averaged Mass-loss Rates of Red Supergiants as Revealed by Their Luminosity Functions in M31 and M33
Philip Massey, Kathryn F. Neugent, Sylvia Ekström, Cyril Georgy and Georges Meynet The Astrophysical Journal 942(2) 69 (2023) https://doi.org/10.3847/1538-4357/aca665
Observing the mass-loss of nearby red supergiants through high-contrast imaging
Peter Scicluna, R. Siebenmorgen, J. A. D. L. Blommaert, et al. Proceedings of the International Astronomical Union 14(S343) 500 (2018) https://doi.org/10.1017/S1743921318007421
A high-contrast imaging survey of nearby red supergiants
Peter Scicluna, Ralf Siebenmorgen, Joris Blommaert, et al. Proceedings of the International Astronomical Union 12(S329) 166 (2016) https://doi.org/10.1017/S1743921317003350
The evolution of red supergiants to supernova in NGC 2100