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Stellar_flare_hits_HD_189733_b_(artist's_impression)

This artist's impression shows the hot Jupiter HD 189733b, as it passes in front of its parent star, as the latter is flaring, driving material away from the planet. The escaping atmosphere is seen silhouetted against the starlight. The surface of the star, which is around 80% the mass of the Sun, is based on observations of the Sun from NASA's Solar Dynamics Observatory.

Credit: NASA, ESA, L. Calçada, Solar Dynamics Observatory

Prof Suzanne Aigrain

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics
  • Exoplanets and planetary physics

Sub department

  • Astrophysics

Research groups

  • Exoplanets and Stellar Physics
Suzanne.Aigrain@physics.ox.ac.uk
Telephone: 01865 (2)73339
Denys Wilkinson Building, room 762
Stars & Planets @ Oxford research group website
  • About
  • Publications

Transiting exoplanets from the CoRoT space mission: XV. CoRoT-15b: A brown-dwarf transiting companion

Astronomy and Astrophysics 525:19 (2011)

Authors:

F Bouchy, M Deleuil, T Guillot, S Aigrain, L Carone, WD Cochran, JM Almenara, R Alonso, M Auvergne, A Baglin, P Barge, AS Bonomo, P Bordé, S Csizmadia, K De Bondt, HJ Deeg, RF Díaz, R Dvorak, M Endl, A Erikson, S Ferraz-Mello, M Fridlund, D Gandolfi, JC Gazzano, N Gibson, M Gillon, E Guenther, A Hatzes, M Havel, G Hébrard, L Jorda, A Léger, C Lovis, A Llebaria, H Lammer, PJ MacQueen, T Mazeh, C Moutou, A Ofir, M Ollivier, H Parviainen, M Pätzold, D Queloz, H Rauer, D Rouan, A Santerne, J Schneider, B Tingley, G Wuchterl

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. © ESO, 2010. © 2010 ESO.

Transiting exoplanets from the CoRoT space mission. XV. CoRoT-15b: a brown-dwarf transiting companion

åp 525 (2011) A68-A68

Authors:

F Bouchy, M Deleuil, T Guillot, S Aigrain, L Carone, WD Cochran, JM Almenara, R Alonso, M Auvergne, A Baglin, P Barge, AS Bonomo, P Bordé, S Csizmadia, K de Bondt, HJ Deeg, RF Díaz, R Dvorak, M Endl, A Erikson, S Ferraz-Mello, M Fridlund, D Gandolfi, JC Gazzano, N Gibson, M Gillon, E Guenther, A Hatzes, M Havel, G Hébrard, L Jorda, A Léger, C Lovis, A Llebaria, H Lammer, PJ MacQueen, T Mazeh, C Moutou, A Ofir, M Ollivier, H Parviainen, M Pätzold, D Queloz, H Rauer, D Rouan, A Santerne, J Schneider, B Tingley, G Wuchterl
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A simple method to estimate radial velocity variations due to stellar activity using photometry

Monthly Notices of the Royal Astronomical Society (2011)

Authors:

S Aigrain, F Pont, S Zucker
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Details from ArXiV

ASTEP: Towards the detection and characterization of exoplanets from Dome C

DETECTION AND DYNAMICS OF TRANSITING EXOPLANETS 11 (2011) ARTN 06001

Authors:

N Crouzet, T Guillot, K Agabi, J-B Daban, L Abe, D Mekarnia, J-P Rivet, Y Fantei-Caujolle, F Fressin, C Gouvret, F-X Schmider, F Valbousquet, A Blazit, H Rauer, A Erikson, T Fruth, S Aigrain, F Pont, M Barbieri
More details from the publisher

ASTEP: Towards the detection and characterization of exoplanets from Dome C

EPJ Web of Conferences EDP Sciences 11 (2011) 06001

Authors:

N Crouzet, T Guillot, K Agabi, J-B Daban, L Abe, D Mekarnia, J-P Rivet, Y Fanteï-Caujolle, F Fressin, C Gouvret, F-X Schmider, F Valbousquet, A Blazit, H Rauer, A Erikson, T Fruth, S Aigrain, F Pont, M Barbieri
More details from the publisher

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