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Temple, LY, Hellier, C, Almleaky, Y, Anderson, DR, Bouchy, F, Brown, DJA, Burdanov, A, Cameron, AC, Delrez, L, Gillon, M, Jehin, E, Lendl, M, Maxted, PFL, Murray, C, Nielsen, LD, Pepe, F, Pollacco, D, Queloz, D, Ségransan, D, Smalley, B, Thompson, S, Triaud, AHMJ, Turner, OD, Udry, S and West, RG (2019) WASP-190b: Tomographic discovery of a transiting hot Jupiter. Astronomy & Astrophysics, 157 (4). ISSN 0004-6361
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Abstract
We report the discovery of WASP-190b, an exoplanet on a 5.37 day orbit around a mildly evolved F6 IV-V star with V = 11.7, = 6400 ± 100 K, M* = 1.35 ± 0.05 M⊙, and R* = 1.6 ± 0.1 R⊙. The planet has a radius of RP = 1.15 ± 0.09 RJup and a mass of MP = 1.0 ± 0.1 MJup, making it a mildly inflated hot Jupiter. It is the first hot Jupiter confirmed via Doppler tomography with an orbital period of >5 days. The orbit is also marginally misaligned with respect to the stellar rotation, with λ = 21° ± 6° measured using Doppler tomography.
Item Type: | Article |
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Additional Information: | This is the final published version of the article (version of record). It first appeared online via EDP Sciences at https://doi.org/10.3847/1538-3881/ab095a - please refer to any applicable terms of use of the publisher. |
Uncontrolled Keywords: | planets and satellites, detection, individual (WASP-190b), stars, (WASP-190) |
Subjects: | Q Science > QB Astronomy > QB460 Astrophysics Q Science > QB Astronomy > QB600 Planets. Planetology Q Science > QB Astronomy > QB799 Stars |
Divisions: | Faculty of Natural Sciences > School of Chemical and Physical Sciences |
Related URLs: | |
Depositing User: | Symplectic |
Date Deposited: | 28 Mar 2019 10:06 |
Last Modified: | 01 Apr 2019 07:58 |
URI: | https://eprints.keele.ac.uk/id/eprint/6117 |