The red-giant CoRoT target HR 7349
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.
- Publication:
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Astrophysics and Space Science
- Pub Date:
- July 2010
- DOI:
- 10.1007/s10509-009-0171-y
- Bibcode:
- 2010Ap&SS.328...83C
- Keywords:
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- Stars: oscillations;
- Stars: variables;
- Stars: interiors