Temple, LY, Hellier, C ORCID: https://orcid.org/0000-0002-3439-1439, Almleaky, Y, Anderson, DR, Bouchy, F, Brown, DJA, Burdanov, A, Cameron, AC, Delrez, L, Gillon, M, Jehin, E, Lendl, M, Maxted, PFL ORCID: https://orcid.org/0000-0003-3794-1317, Murray, C, Nielsen, LD, Pepe, F, Pollacco, D, Queloz, D, Ségransan, D, Smalley, B ORCID: https://orcid.org/0000-0002-3456-087X, 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).

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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
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: http://eprints.keele.ac.uk/id/eprint/6117

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