WASP-104b and WASP-106b : two transiting hot Jupiters in 1.75-day and 9.3-day orbits

Autor: Barry Smalley, François Bouchy, Guillaume Montagnier, J. W. Rostron, Monika Lendl, Francesca Faedi, Y. Gómez Maqueo Chew, Oliver Turner, Didier Queloz, H. P. Osborn, Emmanuel Jehin, Richard G. West, Duncan A. Brown, Michaël Gillon, Don Pollacco, Aldo S. Bonomo, David R. Anderson, Pierre F. L. Maxted, S. C. C. Barros, M. Neveu-VanMalle, Amaury H. M. J. Triaud, Susan Walker, Alexis M. S. Smith, Stéphane Udry, A. Collier Cameron, Francesco Pepe, Damien Ségransan, Tom Louden, Laetitia Delrez, David J. Armstrong, Guillaume Hébrard, Peter J. Wheatley

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2014, 570, ⟨10.1051/0004-6361/201424752⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2014, 570, ⟨10.1051/0004-6361/201424752⟩
Astronomy & Astrophysics

We report the discovery from the WASP survey of two exoplanetary systems, each consisting of a Jupiter-sized planet transiting an 11th magnitude (V) main-sequence star. WASP-104b orbits its star in 1.75 d, whereas WASP-106b has the fourth-longest orb

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96a1100e29cb0671c3559633dfabc2b5
https://hdl.handle.net/10023/5928