The convective surface of the red supergiant Antares. VLTI/PIONIER interferometry in the near infrared
The convective surface of the red supergiant Antares. VLTI/PIONIER interferometry in the near infrared
Context. Convection is a candidate to explain the trigger of red supergiant star mass loss. Owing to the small size of the convective cells on the photosphere, few of their characteristics are known. Aims. Using near infrared interferometry, we intend to resolve the photosphere of red supergiant stars and to …