SIMBAD references

2019MNRAS.485.5790T - Mon. Not. R. Astron. Soc., 485, 5790-5799 (2019/June-1)

Three hot-Jupiters on the upper edge of the mass-radius distribution: WASP-177, WASP-181, and WASP-183.

TURNER O.D., ANDERSON D.R., BARKAOUI K., BOUCHY F., BENKHALDOUN Z., BROWN D.J.A., BURDANOV A., COLLIER CAMERON A., DUCROT E., GILLON M., HELLIER C., JEHIN E., LENDL M., MAXTED P.F.L., NIELSEN L.D., PEPE F., POLLACCO D., POZUELOS F.J., QUELOZ D., SEGRANSAN D., SMALLEY B., TRIAUD A.H.M.J., UDRY S. and WEST R.G.

Abstract (from CDS):

We present the discovery of three transiting planets from the WASP survey, two hot-Jupiters: WASP-177 b (∼0.5 MJup, ∼1.6 RJup) in a 3.07-d orbit of a V = 12.6 K2 star, WASP-183 b (∼0.5 MJup, ∼1.5 RJup) in a 4.11-d orbit of a V = 12.8 G9/K0 star; and one hot-Saturn planet WASP-181 b (∼0.3 MJup, ∼1.2 RJup) in a 4.52-d orbit of a V = 12.9 G2 star. Each planet is close to the upper bound of mass-radius space and has a scaled semimajor axis, a/R*, between 9.6 and 12.1. These lie in the transition between systems that tend to be in orbits that are well aligned with their host-star's spin and those that show a higher dispersion.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): planets and satellites: detection - planets and satellites: individual: WASP-177b - planets and satellites: individual: WASP-181b - planets and satellites: individual: WASP-183b

VizieR on-line data: <Available at CDS (J/MNRAS/485/5790): table3.dat tablea1.dat tablea2.dat tablea3.dat tablea4.dat>

Simbad objects: 12

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