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arXiv · 1111.4366

Solar-like pulsating stars as distance indicators: G-K giants in the CoRoT and Kepler fields

Andrea Miglio·Thierry Morel·Mauro Barbieri·Benoit Mosser·Leo Girardi·Josefina Montalban·Marica Valentini
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Abstract

The detection of radial and non-radial solar-like oscillations in thousands of G-K giants with CoRoT and Kepler is paving the road for detailed studies of stellar populations in the Galaxy. The available average seismic constraints allow a precise and largely model-independent determination of stellar radii (hence distances) and masses. We here briefly report on the distance determination of thousands of giants in the CoRoT and Kepler fields of view.

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Andrea Miglio, Thierry Morel, Mauro Barbieri, Benoit Mosser, Leo Girardi, Josefina Montalban, Marica Valentini. 2011-11-18. Solar-like pulsating stars as distance indicators: G-K giants in the CoRoT and Kepler fields. https://doi.org/10.1051/epjconf%2F20121905012

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