Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2010-10-14
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
As accepted for publication in ApJL (6 pages, 2 figures, 3 tables)
Scientific paper
We report the discovery of a 61-Jupiter-mass brown dwarf, which transits its F8V host star, WASP-30, every 4.16 days. From a range of age indicators we estimate the system age to be 1-2 Gyr. We derive a radius (0.89 +/- 0.02 RJup) for the companion that is consistent with that predicted (0.914 RJup) by a model of a 1-Gyr-old, non-irradiated brown dwarf with a dusty atmosphere. The location of WASP-30b in the minimum of the mass-radius relation is consistent with the quantitative prediction of Chabrier & Baraffe (2000), thus confirming the theory.
Anderson David R.
Barros S. C. C.
Collier Cameron Andrew
Enoch B.
Gillon Michael
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