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24 April 2024
 
  » arxiv » 1704.7771

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WASP-167b/KELT-13b: Joint discovery of a hot Jupiter transiting a rapidly-rotating F1V star
L.Y. Temple ; C. Hellier ; 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 ; P.F.L. Maxted ; G. Myers ; T. E. Oberst ; F. Pepe ; J. Pepper ; D. Pollacco ; D. Queloz ; J. E. Rodriguez ; D. Ségransan ; R. J. Siverd ; B. Smalley ; 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 ;
Date 25 Apr 2017
AbstractWe 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 $pm$ 0.1. The 1.5 R$_{ m Jup}$ planet was confirmed by Doppler tomography of the stellar line profiles during transit. We place a limit of $<$ 8 M$_{ m Jup}$ on its mass. The planet is in a retrograde orbit with a sky-projected spin-orbit angle of $lambda = -165^{circ} pm 5^{circ}$. 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 $delta$-Scuti or $gamma$-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.
Source arXiv, 1704.7771
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