WASP-103 b: a new planet at the edge of tidal disruption

M. Gillon; D. R. Anderson; A. Collier-Cameron; L. Delrez; C. Hellier; E. Jehin; M. Lendl; P. F. L. Maxted; F. Pepe; D. Pollacco; D. Queloz; D. Ségransan; A. M. S. Smith; B. Smalley; J. Southworth; A. H. M. J. Triaud; S. Udry; V. Van Grootel; R. G. West

doi:10.1051/0004-6361/201323014

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Volume 562 (February 2014)

A&A, 562 (2014) L3

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Fig. 4

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Diagram planetary mass vs. orbital distance to Roche-limit ratio for known transiting hot Jupiters (M > 0.2M_Jup, P < 12 d; data from NASA Exoplanet Archive). O56=OGLE-TR-56 b, W12=WASP-12 b, W19=WASP-19 b, and W103=WASP-103 b. Here we only show planets with a ratio of the orbital distance to the Roche-limit lower than 2.5.

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