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.
@article{arxiv.2001.03497,
title = {The prototype star $\gamma$ Doradus observed by TESS},
author = {S. Christophe and V. Antoci and E. Brunsden and R. -M. Ouazzani and S. J. A. J. Salmon},
journal= {arXiv preprint arXiv:2001.03497},
year = {2020}
}
Comments
2 pages, 2 figures, poster contribution at the conference "Stars and their variability observed from space - Celebrating the 5th anniversary of BRITE-Constellation", Vienna, Austria, August 19 - 23, 2019. Eds: C. Neiner, W. Weiss, D. Baade, E. Griffin, C. Lovekin, A. Moffat