WASP-113b and WASP-114b, two inflated hot Jupiters with contrasting densities

Autor: D. L. Pollacco, D. Queloz, J. McCormac, L. Delrez, Richard G. West, S. R. Walker, Isabelle Boisse, François Bouchy, Emmanuel Jehin, Francesca Faedi, Brian A. Skiff, A. Collier Cameron, Michaël Gillon, P. J. Wheatley, David J. Armstrong, M. Vanhuysse, Christopher A. Watson, Oliver Turner, Monika Lendl, Stéphane Udry, G. Hebrard, Barry Smalley, A. H. M. J. Triaud, P. Boumis, I. Plauchu-Frayn, C. Hellier, Y. Gómez Maqueo Chew, David R. Anderson, Jessica Spake, S. C. C. Barros, K. W. F. Lam, John Meaburn, Hugh P. Osborn, Duncan A. Brown, D. Segransan, K. L. Hay, Joe Llama, Alexios Liakos, Francesco Pepe, J. Rey

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2016, 593, ⟨10.1051/0004-6361/201526517⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 593, ⟨10.1051/0004-6361/201526517⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 593, 〈10.1051/0004-6361/201526517〉

International audience; Aims. We present the discovery and characterisation of the exoplanets WASP-113b and WASP-114b by the WASP surveys, SOPHIE and CORALIE. Methods. The planetary nature of the systems was established by performing follow-up photom

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a7613a0c6f1a6d9829e25fde7c0afe5
https://hal.science/hal-01441173/document