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The convection of close red supergiant stars observed with near-infrared interferometry

Abstract

Our team has obtained observations of the photosphere of the two closest red supergiant stars Betelgeuse (α\alpha Ori) and Antares (α\alpha Sco) using near infrared interferometry. We have been monitoring the photosphere of Betelgeuse with the VLTI/PIONIER instrument for three years. On Antares, we obtained an unprecedented sampling of the visibility function. These data allow us to probe the convective photosphere of massive evolved stars.Comment: 5 pages, 3 figures. Published in the proceedings of the Physics Of Evolved Stars conference, dedicated to the memory of Olivier Chesneau (Nice, France, 2015

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