Analysis of rotation and stochastic variability of CoRoT dwarf stars

Details Analysis of rotation and stochastic variability of CoRoT dwarf stars Analysis of rotation and stochastic variability of CoRoT dwarf stars

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1094..341a&link_type=abstract

COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun.

Statistics

1

Low Luminosity Stars, Subdwarfs, And Brown Dwarfs, Photometric, Polarimetric, And Spectroscopic Instrumentation, Pulsations, Oscillations, And Stellar Seismology

Scientific paper

We study the distribution and evolution of rotational periods in field solar-type stars, using the light curves (LCs) produced by CoRoT. The large number of CoRoT targets at our disposal allows us to perform this study on a statistically representative sample, and therefore to investigate the statistics of variability (i.e. flares, starspots) in stellar samples differing for example in terms of activity, age and mass, and focusing, in particular, on the analysis of the young population's properties in the solar neighbourhood. This work is based on a CoRoT additional program (P.I. Fabio Favata).

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