Carrier, Fabien × Morel, T Miglio, A Montalban, J Auvergne, M Baglin, A Baudin, F Barban, C Catala, C D'Antona, F De Ridder, Joris Eggenberger, P Hatzes, A. P Hekker, S Kallinger, T Michel, E Noels, A Poretti, E Rainer, M Samadi, R Ventura, P Weiss, W. W #
Astrophysics and space science vol:328 issue:1-2 pages:83-86
HR 7349 is a bright [V = 5.8] red giant observed by CoRoT in the seismofield of the first long run. The outstanding CoRoT light curve allowed the detection of several solar-like oscillation modes (both radial and non-radial). On top of these seismic constraints, our observational knowledge on HR 7349 benefits as well from a precise parallax and detailed spectroscopic constraints. We present all the observational constraints that are available for the theoretical modelling of this most promising target.