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Paper detail

The prototype star $γ$ Doradus observed by TESS

$γ$ Doradus is the prototype star for the eponymous class of pulsating stars that consists of late A-early F main-sequence stars oscillating in low-frequency gravito-inertial modes. Being among the brightest stars of its kind (V = 4.2), $γ$ Dor benefits from a large set of observational data that has been recently completed by high-quality space photometry from the TESS mission. With these new data, we propose to study $γ$ Dor as an example of possibilities offered by synergies between multi-technical ground and space-based observations. Here, we present the preliminary results of our investigations.

preprint2020arXivOpen access
S. ChristopheV. AntociE. BrunsdenR. -M. OuazzaniS. J. A. J. Salmon
astro-ph.SR
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S. ChristopheV. AntociE. BrunsdenR. -M. OuazzaniS. J. A. J. Salmon

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