# The convective photosphere of the red supergiant CE Tauri

@article{Montargs2018TheCP,
title={The convective photosphere of the red supergiant CE Tauri},
author={Miguel Montarg{\e}s and Ray P. Norris and Andrea Chiavassa and B. Tessore and A. L{\e}bre and Fabien R. Baron},
journal={Astronomy \& Astrophysics},
year={2018}
}
• Published 16 February 2018
• Physics
• Astronomy & Astrophysics
Context. Red supergiant stars are one of the latest stages in the evolution of massive stars. Their photospheric convection may play an important role in the launching mechanism of their mass loss; however, its characteristics and dynamics are still poorly constrained. Aims. By observing red supergiant stars with near infrared interferometry at different epochs, we expect to reveal the evolution of bright convective features on their stellar surface. Methods. We observed the M2Iab-Ib red…
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