Abstract
We report the discovery by the CoRoT space mission of a transiting brown dwarf orbiting a F7V star with an orbital period of 3.06 days. CoRoT-15b has a radius of 1.12+0.30-0.15 RJup and a mass of 63.3 ± 4.1 MJup, and is thus the second transiting companion lying in the theoretical mass domain of brown dwarfs. CoRoT-15b is either very young or inflated compared to standard evolution models, a situation similar to that of M-dwarf stars orbiting close to solar-typestars. Spectroscopic constraints and an analysis of the lightcurve imply a spin period in the range 2.9-3.1 days for the central star, which is compatible with a double-synchronisation of the system.
Original language | English |
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Article number | A68 |
Journal | Astronomy and Astrophysics |
Volume | 525 |
Issue number | 19 |
State | Published - Jan 2011 |
Keywords
- Brown dwarfs
- Planetary systems
- Stars: low-mass
- Techniques: photometric
- Techniques: radial velocities
- Techniques: spectroscopic