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.
| Original language | English |
|---|---|
| Journal | Astrophysics and Space Science |
| DOIs | |
| Publication status | Published - 20 Oct 2009 |
Keywords
- Stars: variables
- Stars: oscillations
- Stars: interiors
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