Context. Asymptotic giant branch (AGB) stars are characterised by complex stellar surface dynamics that affect the measurements and amplify the uncertainties on stellar parameters. The uncertainties in observed absolute magnitudes have been found to originate mainly from uncertainties in the parallaxes. The resulting motion of the stellar...
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September 2018 (v1)Journal articleUploaded on: December 4, 2022
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May 2022 (v1)Journal article
Context. Red supergiant (RSGs) are cool massive stars in a late phase of their evolution when the stellar envelope becomes fully convective. They are the brightest stars in the universe at infrared light and can be detected in galaxies far beyond the Local Group, allowing for accurate determination of chemical composition of galaxies. The study...
Uploaded on: December 3, 2022 -
February 2018 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
October 9, 2019 (v1)Journal article
Red supergiants are cool massive stars and are the largest and the most luminous stars in the universe. They are characterized by irregular or semi-regular photometric variations, the physics of which is not clearly understood. The paper aims at deriving the velocity field in the red supergiant star μ Cep and relating it to the photometric...
Uploaded on: December 3, 2022 -
April 1, 2021 (v1)Journal article
Despite being the best studied red supergiant star in our Galaxy, the physics behind the photometric variability and mass loss of Betelgeuse is poorly understood. Moreover, recently the star has experienced an unusual fading with its visual magnitude reaching a historical minimum. We investigate the nature of this event with the help of a...
Uploaded on: December 3, 2022 -
February 25, 2020 (v1)Journal article
Context. Red supergiant stars possess surface features and extended molecular atmospheres. Photospheric convection may be a crucial factor of the levitation of the outer atmospheric layers. However, the mechanism responsible is still poorly understood. Aims. We image the stellar surface of V602 Carinae (V602 Car) to constrain the morphology and...
Uploaded on: December 4, 2022 -
2011 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
January 2018 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
2020 (v1)Journal article
Context. Asymptotic giant branch (AGB) stars are cool luminous evolved stars that are well observable across the Galaxy and populating Gaia data. They have complex stellar surface dynamics, which amplifies the uncertainties on stellar parameters and distances.Aims. On the AGB star CL Lac, it has been shown that the convection-related...
Uploaded on: December 4, 2022 -
2010 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
2022 (v1)Journal article
Context. VX Sgr is a cool, evolved, and luminous red star whose stellar parameters are difficult to determine, which affects its classification.Aims. We aim to spatially resolve the photospheric extent as well as the circumstellar environment.Methods. We used interferometric observations obtained with the MATISSE instrument in the L (3–4 μm), M...
Uploaded on: December 3, 2022