Transiting exoplanets from the CoRoT space mission. XXI. CoRoT-19b: a low density planet orbiting an old inactive F9V-star

@article{Guenther2011TransitingEF,
  title={Transiting exoplanets from the CoRoT space mission. XXI. CoRoT-19b: a low density planet orbiting an old inactive F9V-star},
  author={E. W. Guenther and Rodrigo F. D{\'i}az and J. C. Gazzano and Tsevi Mazeh and Daniel Rouan and Neale P. Gibson and Sz. Csizmadia and Suzanne Aigrain and Roi Alonso and Jose M. Almenara and Michel Auvergne and Annie Baglin and Pierre Barge and Aldo Stefano Bonomo and Pascal J. Bord{\'e} and François Bouchy and Hans Bruntt and J. Cabrera and Ludmila Carone and Stefania Carpano and C{\'e}line Cavarroc and Hans J. Deeg and Magali Deleuil and Stefan Dreizler and Rudolf Dvorak and Anders Erikson and Sylvio Ferraz-Mello and Malcolm Fridlund and Davide Gandolfi and Micha{\"e}l Gillon and Tristan Guillot and A. P. Hatzes and Mathieu Havel and Guillaume H{\'e}brard and Emmanuel Jehin and Laurent Jorda and Helmut Lammer and Alain L{\'e}ger and Claire Moutou and Lisa Nortmann and Marc Ollivier and Aviv Ofir and Th. Pasternacki and Martin Paetzold and Hannu Parviainen and Didier Queloz and Heike Rauer and Benjamin Samuel and Alexandre Santerne and Jodi Schneider and L. Tal-Or and Brandon Tingley and Joerg Weingrill and G{\"u}nther Wuchterl},
  journal={Astronomy and Astrophysics},
  year={2011},
  volume={537}
}
Context. Observations of transiting extrasolar planets are of key importance to our understanding of planets because their mass, radius, and mass density can be determined. These measurements indicate that planets of similar mass can have very di erent radii. For low-density planets, it is generally assumed that they are inflated owing to their proximity to the host-star. To determine the causes of this inflation, it is necessary to obtain a statistically significant sample of planets with… 

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