Rossiter-McLaughlin effect measurements for WASP-16, WASP-25 and WASP-31

D.~J.~A. Brown, A.~C. Cameron, D.~R. Anderson, B. Enoch, C. Hellier, P.~F.~L. Maxted, G.~R.~M. Miller, D. Pollacco, D. Queloz, E. Simpson, B. Smalley, A.~H.~M.~J. Triaud, I. Boisse, F. Bouchy, M. Gillon, G. Hébrard

Research output: Contribution to journalArticlepeer-review

28 Citations (Scopus)

Abstract

We present new measurements of the Rossiter–McLaughlin (RM) effect for three Wide Angle Search for transiting Planets (WASP) planetary systems, WASP-16, WASP-25 and WASP-31, from a combined analysis of their complete sets of photometric and spectroscopic data. We find a low-amplitude RM effect for WASP-16 (Teff= 5700 ± 150 K), suggesting that the star is a slow rotator and thus of an advanced age, and obtain a projected alignment angle of Graphic. For WASP-25 (Teff= 5750 ± 100 K), we detect a projected spin–orbit angle of λ= 14°.6 ± 6°.7. WASP-31 (Teff= 6300 ± 100 K) is found to be well aligned, with a projected spin–orbit angle of λ= 2°.8 ± 3°.1. A circular orbit is consistent with the data for all three systems, in agreement with their respective discovery papers. We consider the results for these systems in the context of the ensemble of RM measurements made to date. We find that whilst WASP-16 fits the hypothesis of Winn et al. that ‘cool’ stars (Teff < 6250 K) are preferentially aligned, WASP-31 has little impact on the proposed trend. We bring the total distribution of the true spin–orbit alignment angle, ψ, up to date, noting that recent results have improved the agreement with the theory of Fabrycky & Tremaine at mid-range angles. We also suggest a new test for judging misalignment using the Bayesian information criterion, according to which WASP-25 b’s orbit should be considered to be aligned.
Original languageEnglish
Pages (from-to)1503-1520
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume423
Issue number2
DOIs
Publication statusPublished - 21 Jun 2012

Fingerprint

Dive into the research topics of 'Rossiter-McLaughlin effect measurements for WASP-16, WASP-25 and WASP-31'. Together they form a unique fingerprint.
  • RV curves of WASP-16, 25 and 31 (Brown+, 2012)

    Brown, D. J. A. (Creator), Cameron, A. C. (Creator), Anderson, D. R. (Creator), Enoch, R. L. (Creator), Hellier, C. (Creator), Maxted, P. F. L. (Creator), Miller, G. R. M. (Creator), Pollacco, D. (Creator), Queloz, D. (Creator), Simpson, E. (Creator), Smalley, B. (Creator), Triaud, A. H. M. J. (Creator), Boisse, I. (Creator), Bouchy, F. (Creator), Gillon, M. (Creator) & Hebrard, G. (Creator), Strasbourg astronomical Data Center, 1 Apr 2013

    Dataset

Cite this