Coel Hellier c.hellier@keele.ac.uk
Three WASP-South transiting exoplanets: WASP-74b, WASP-83b & WASP-89b
Hellier, Coel; Anderson, D.R.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Jehin, E.; Lendl, M.; Maxted, Pierre; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, Barry; Smith, A.M.S.; Southworth, John; Triaud, A.H.M.J.; Turner, O.D.; Udry, S.; West, R.G.
Authors
D.R. Anderson
A. Collier Cameron
L. Delrez
M. Gillon
E. Jehin
M. Lendl
Pierre Maxted p.maxted@keele.ac.uk
F. Pepe
D. Pollacco
D. Queloz
D. Ségransan
Barry Smalley b.smalley@keele.ac.uk
A.M.S. Smith
Dr John Taylor j.k.taylor@keele.ac.uk
A.H.M.J. Triaud
O.D. Turner
S. Udry
R.G. West
Abstract
We report the discovery of three new transiting hot Jupiters by WASP-South together with the TRAPPIST photometer and the Euler/CORALIE spectrograph. WASP-74b orbits a star of V = 9.7, making it one of the brighter systems accessible to Southern telescopes. It is a 0.95 M_Jup planet with a moderately bloated radius of 1.5 R_Jup in a 2-d orbit around a slightly evolved F9 star. WASP-83b is a Saturn-mass planet at 0.3 M_Jup with a radius of 1.0 R_Jup. It is in a 5-d orbit around a fainter (V = 12.9) G8 star. WASP-89b is a 6 M_Jup planet in a 3-d orbit with an eccentricity of e = 0.2. It is thus similar to massive, eccentric planets such as XO-3b and HAT-P-2b, except that those planets orbit F stars whereas WASP-89 is a K star. The V = 13.1 host star is magnetically active, showing a rotation period of 20.2 d, while star spots are visible in the transits. There are indications that the planet's orbit is aligned with the stellar spin. WASP-89 is a good target for an extensive study of transits of star spots.
Citation
Hellier, C., Anderson, D., Collier Cameron, A., Delrez, L., Gillon, M., Jehin, E., …West, R. (2014). Three WASP-South transiting exoplanets: WASP-74b, WASP-83b & WASP-89b. Astronomical Journal, 150(1), Article 18. https://doi.org/10.1088/0004-6256/150/1/18
Journal Article Type | Article |
---|---|
Acceptance Date | May 7, 2015 |
Online Publication Date | Jun 24, 2015 |
Publication Date | Oct 23, 2014 |
Journal | Astronomical Journal |
Print ISSN | 0004-6256 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 150 |
Issue | 1 |
Article Number | 18 |
DOI | https://doi.org/10.1088/0004-6256/150/1/18 |
Keywords | astrophysics; planetary systems; stars; WASP74; WASP83; WASP89 |
Publisher URL | http://arxiv.org/abs/1410.6358v2 |
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