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WASP-South hot Jupiters: WASP-178b, WASP-184b, WASP-185b & WASP-192b

Smalley; Hellier; Maxted

WASP-South hot Jupiters: WASP-178b, WASP-184b, WASP-185b & WASP-192b Thumbnail


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Abstract

We report on four new transiting hot Jupiters discovered by the WASP-South survey. WASP-178b transits a V = 9.9, A1V star with Teff = 9350 ± 150 K, the second-hottest transit host known. It has a highly bloated radius of 1.81 ± 0.09 RJup, in line with the known correlation between high irradiation and large size. With an estimated temperature of 2470 ± 60 K, the planet is one of the best targets for studying ultra-hot Jupiters that is visible from the Southern hemisphere. The three host stars WASP-184, WASP-185 and WASP-192 are all post-main-sequence G0 stars of ages 4–8 Gyr. The larger stellar radii (1.3–1.7 M?) mean that the transits are relatively shallow (0.7–0.9%) even though the planets have moderately inflated radii of 1.2–1.3 RJup. WASP-185b has an eccentric orbit (e = 0.24) and a relatively long orbital period of 9.4 d. A star that is 4.6 arcsec from WASP-185 and 4.4 mag fainter might be physically associated.

Acceptance Date Sep 29, 2019
Publication Date Nov 1, 2019
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Publisher Oxford University Press
Pages 1479-1487
DOI https://doi.org/10.1093/mnras/stz2713
Keywords stars: individual: WASP-178, stars: individual: WASP-184, stars: individual: WASP-185, stars: individual: WASP-192, planetary systems
Publisher URL https://doi.org/10.1093/mnras/stz2713

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