Author
Listed:
- J. F. Donati
(Université de Toulouse, UPS-OMP, IRAP
Centre National de la Recherche Scientifique (CNRS), IRAP/UMR 5277)
- C. Moutou
(Canada–France–Hawaii Telescope (CFHT) Corporation, 65-1238 Mamalahoa Highway)
- L. Malo
(Canada–France–Hawaii Telescope (CFHT) Corporation, 65-1238 Mamalahoa Highway)
- C. Baruteau
(Université de Toulouse, UPS-OMP, IRAP
Centre National de la Recherche Scientifique (CNRS), IRAP/UMR 5277)
- L. Yu
(Université de Toulouse, UPS-OMP, IRAP
Centre National de la Recherche Scientifique (CNRS), IRAP/UMR 5277)
- E. Hébrard
(York University)
- G. Hussain
(European Southern Observatory (ESO), Karl-Schwarzschild-Strasse 2)
- S. Alencar
(ICEx, UFMG)
- F. Ménard
(Université Grenoble Alpes, IPAG, BP 53
CNRS, IPAG/UMR 5274, BP 53)
- J. Bouvier
(Université Grenoble Alpes, IPAG, BP 53
CNRS, IPAG/UMR 5274, BP 53)
- P. Petit
(Université de Toulouse, UPS-OMP, IRAP
Centre National de la Recherche Scientifique (CNRS), IRAP/UMR 5277)
- M. Takami
(Institute of Astronomy and Astrophysics, Academia Sinica)
- R. Doyon
(Départment de physique, Université de Montréal, CP 6128, Succursale Centre-Ville)
- A. Collier Cameron
(SUPA, School of Physics and Astronomy, University of St Andrews)
Abstract
The radial velocities of a young star are measured, revealing the presence of a planet of mass about three-quarters that of Jupiter, orbiting its host star very closely, and thus demonstrating that ‘hot Jupiters’ can migrate inwards in less than two million years.
Suggested Citation
J. F. Donati & C. Moutou & L. Malo & C. Baruteau & L. Yu & E. Hébrard & G. Hussain & S. Alencar & F. Ménard & J. Bouvier & P. Petit & M. Takami & R. Doyon & A. Collier Cameron, 2016.
"A hot Jupiter orbiting a 2-million-year-old solar-mass T Tauri star,"
Nature, Nature, vol. 534(7609), pages 662-666, June.
Handle:
RePEc:nat:nature:v:534:y:2016:i:7609:d:10.1038_nature18305
DOI: 10.1038/nature18305
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