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arXiv · 1603.07597

Exploration of the brown dwarf regime around solar-like stars by CoRoT

Szilárd Csizmadia
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Abstract

Aims. A summary of the CoRoT brown dwarf investigations are presented. Methods. Transiting brown dwarfs around solar like stars were studied by using the photometric time-series of CoRoT, and ground based radial velocity measurements. Results. CoRoT detected three transiting brown dwarfs around F and G dwarf stars. The occurence rate of brown dwarfs was found to be 0.20 +/- 0.15% around solar-like stars which is compatible with the value obtained by Kepler-data.

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Szilárd Csizmadia. 2016-03-24. Exploration of the brown dwarf regime around solar-like stars by CoRoT. https://doi.org/10.1051/978-2-7598-1876-1.c036

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