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Seven transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-47b, WASP-55b, WASP-61b, WASP-62b, WASP-63b, WASP-66b and WASP-67b

WASP-South hot Jupiters

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 20 Sep 2012Embargo end date: 01 Jan 2012 Switzerland, United Kingdom English Publisher:Oxford University Press (OUP)Journal:Monthly Notices of the Royal Astronomical Society, volume 426, pages 739-750 (issn: 0035-8711,

Authors: Hellier, Coel; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, Michael; Jehin, E.; +12 Authors

doi: 10.1111/j.1365-2966.2012.21780.x , 10.48550/arxiv.1204.5095

arXiv: http://arxiv.org/abs/1204.5095

handle: 2381/13984

Seven transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-47b, WASP-55b, WASP-61b, WASP-62b, WASP-63b, WASP-66b and WASP-67b

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Abstract

We present seven new transiting hot Jupiters from the WASP-South survey. The planets are all typical hot Jupiters orbiting stars from F4 to K0 with magnitudes of V = 10.3 to 12.5. The orbital periods are all in the range 3.9--4.6 d, the planetary masses range from 0.4--2.3 Mjup and the radii from 1.1--1.4 Mjup. In line with known hot Jupiters, the planetary densities range from Jupiter-like to inflated (rho = 0.13--1.07 rho_jup). We use the increasing numbers of known hot Jupiters to investigate the distribution of their orbital periods and the 3--4-d "pile-up".

15 pages

Countries

Switzerland, United Kingdom

Related Organizations

University of Liège
Belgium
University of Geneva
Switzerland
University of Leicester
United Kingdom
Centre for Research in Astrophysics of Québec
Canada
Keele University
United Kingdom

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Keywords

Earth and Planetary Astrophysics (astro-ph.EP), FOS: Physical sciences, 520, Planetary systems, Astrophysics - Earth and Planetary Astrophysics, ddc: ddc:520

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