The red-giant CoRoT target HR 7349

Details The red-giant CoRoT target HR 7349 The red-giant CoRoT target HR 7349

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ap%26ss.328...83c&link_type=abstract

Astrophysics and Space Science, Volume 328, Issue 1-2, pp. 83-86

Astronomy and Astrophysics

Astrophysics

4

Stars: Oscillations, Stars: Variables, Stars: Interiors

Scientific paper

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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