Affiliation
OCA, CEA (Paris) SSI (Boulder)
Main category
Natural Sciences (Astrophysics and Astrononmy)
Abstract
We present stellar properties of 58 stars from a seismic inference using full-length data sets from Kepler (mass, age, radius, distances). These stars comprise active stars, planet-hosts, solar-analogs, and binary systems. By employing the frequency separation ratios, we test the applicability of the Kjeldsen et al (2008) empirical surface correction. Ensemble analyses exhibit interesting trends, for example, with mixing length
parameter or effective temperature. We present ages of binary components and characterize some planetary systems.
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