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Atmosphere tomography of red supergiant stars
EAS Publications Series, 20133-D simulations suggest that the atmospheres of red super-giants are subject to large-amplitude convective motions, which are suspected to generate supersonic motions and shocks. We perform tomography of supergiant-star atmospheres, on temporal series of high-resolution spectra and on 3-D hydrodynamical synthetic spectra.
S. Lion +4 more
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Yellow supergiants as supernova progenitors: an indication of strong mass loss for red supergiants?
Astronomy and Astrophysics, 2012Cyril Georgy
exaly
A new mass-loss rate prescription for red supergiants
Monthly Notices of the Royal Astronomical Society, 2020Emma Beasor, Ben En Davies, Nathan Smith
exaly
Red Supergiants, Yellow Hypergiants, and Post-RSG Evolution
Galaxies, 2019Michael S Gordon, Roberta M Humphreys
exaly
The evolution of red supergiants to supernova in NGC 2100
Monthly Notices of the Royal Astronomical Society, 2016Emma Beasor, Ben En Davies
exaly
An LTE effective temperature scale for red supergiants in the Magellanic clouds
Monthly Notices of the Royal Astronomical Society, 2018Hugo M Tabernero +2 more
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