L.Y. Temple
WASP-167b/KELT-13b: joint discovery of a hot Jupiter transiting a rapidly rotating F1V star
Temple, L.Y.; Hellier, C.; Albrow, M.D.; Anderson, D.R.; Bayliss, D.; Beatty, T.G.; Bieryla, A.; Brown, D.J.A.; Cargile, P.A.; Collier Cameron, A.; Collins, K.A.; Colón, K.D.; Curtis, I.A.; D'Ago, G.; Delrez, L.; Eastman, J.; Gaudi, B.S.; Gillon, M.; Gregorio, J.; James, D.; Jehin, E.; Joner, M.D.; Kielkopf, J.F.; Kuhn, R.B.; Labadie-Bartz, J.; Latham, D.W.; Lendl, M.; Lund, M.B.; Malpas, A.L.; Maxted, P.F.L.; Myers, G.; Oberst, T.E.; Pepe, F.; Pepper, J.; Pollacco, D.; Queloz, D.; Rodriguez, J.E.; Ségransan, D.; Siverd, R.J.; Smalley, B.; Stassun, K.G.; Stevens, D.J.; Stockdale, C.; Tan, T.G.; Triaud, A.H.M.J.; Udry, S.; Villanueva Jr., S.; West, R.G.; Zhou, G.
Authors
Coel Hellier c.hellier@keele.ac.uk
M.D. Albrow
D.R. Anderson
D. Bayliss
T.G. Beatty
A. Bieryla
D.J.A. Brown
P.A. Cargile
A. Collier Cameron
K.A. Collins
K.D. Colón
I.A. Curtis
G. D'Ago
L. Delrez
J. Eastman
B.S. Gaudi
M. Gillon
J. Gregorio
D. James
E. Jehin
M.D. Joner
J.F. Kielkopf
R.B. Kuhn
J. Labadie-Bartz
D.W. Latham
M. Lendl
M.B. Lund
A.L. Malpas
Pierre Maxted p.maxted@keele.ac.uk
G. Myers
T.E. Oberst
F. Pepe
J. Pepper
D. Pollacco
D. Queloz
J.E. Rodriguez
D. Ségransan
R.J. Siverd
Barry Smalley b.smalley@keele.ac.uk
K.G. Stassun
D.J. Stevens
C. Stockdale
T.G. Tan
A.H.M.J. Triaud
S. Udry
S. Villanueva Jr.
R.G. West
G. Zhou
Abstract
We report the joint WASP/KELT discovery of WASP-167b/KELT-13b, a transiting hot Jupiter with a 2.02-d orbit around a V = 10.5, F1V star with [Fe/H] = 0.1 ± 0.1. The 1.5 RJup planet was confirmed by Doppler tomography of the stellar line profiles during transit. We place a limit of <8 MJup on its mass. The planet is in a retrograde orbit with a sky-projected spin–orbit angle of λ = −165° ± 5°. This is in agreement with the known tendency for orbits around hotter stars to be more likely to be misaligned. WASP-167/KELT-13 is one of the few systems where the stellar rotation period is less than the planetary orbital period. We find evidence of non-radial stellar pulsations in the host star, making it a δ-Scuti or γ-Dor variable. The similarity to WASP-33, a previously known hot-Jupiter host with pulsations, adds to the suggestion that close-in planets might be able to excite stellar pulsations.
Citation
Temple, L., Hellier, C., Albrow, M., Anderson, D., Bayliss, D., Beatty, T., …Zhou, G. (2017). WASP-167b/KELT-13b: joint discovery of a hot Jupiter transiting a rapidly rotating F1V star. Monthly Notices of the Royal Astronomical Society, 471(3), 2743 - 2752. https://doi.org/10.1093/mnras/stx1729
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 7, 2017 |
Online Publication Date | Jul 13, 2017 |
Publication Date | 2017-11 |
Publicly Available Date | May 26, 2023 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 471 |
Issue | 3 |
Pages | 2743 - 2752 |
DOI | https://doi.org/10.1093/mnras/stx1729 |
Keywords | techniques, photometric, spectroscopic, planets and satellites, individual, stars, rotation |
Publisher URL | https://academic.oup.com/mnras/article/471/3/2743/3964539 |
Files
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