Abstract
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.
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Carrier, F., Morel, T., Miglio, A. et al. The red-giant CoRoT target HR 7349. Astrophys Space Sci 328, 83–86 (2010). https://doi.org/10.1007/s10509-009-0171-y
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DOI: https://doi.org/10.1007/s10509-009-0171-y