Mon. Not. R. Astron. Soc., 465, 3693-3707 (2017/March-1)
WASP-South transiting exoplanets: WASP-130b, WASP-131b, WASP-132b, WASP-139b, WASP-140b, WASP-141b and WASP-142b.
HELLIER C., ANDERSON D.R., COLLIER CAMERON A., DELREZ L., GILLON M., JEHIN E., LENDL M., MAXTED P.F.L., NEVEU-VANMALLE M., PEPE F., POLLACCO D., QUELOZ D., SEGRANSAN D., SMALLEY B., SOUTHWORTH J., TRIAUD A.H.M.J., UDRY S., WAGG T. and WEST R.G.
Abstract (from CDS):
We describe seven exoplanets transiting stars of brightness V = 10.1-12.4. WASP-130b is a 'warm Jupiter' having an orbital period of 11.6 d around a metal-rich G6 star. Its mass and radius (1.23 ± 0.04 MJup and 0.89 ± 0.03 RJup) support the trend that warm Jupiters have smaller radii than hot Jupiters. WASP-131b is a bloated Saturn-mass planet (0.27 MJup and 1.22 RJup). Its large scaleheight and bright (V = 10.1) host star make it a good target for atmospheric characterization. WASP-132b (0.41 MJup and 0.87 RJup) is among the least irradiated and coolest of WASP planets, having a 7.1-d orbit around a K4 star. WASP-139b is a 'super-Neptune' akin to HATS-7b and HATS-8b, being the lowest mass planet yet found by WASP (0.12 MJup and 0.80 RJup). The metal-rich K0 host star appears to be anomalously dense, akin to HAT-P-11. WASP-140b is a 2.4-MJup planet in an eccentric (e = 0.047 ± 0.004) 2.2-d orbit. The planet's radius is large (1.4 RJup), but uncertain owing to the grazing transit (b = 0.93). The 10.4-d rotation period of the K0 host star suggests a young age, and the time-scale for tidal circularization is likely to be the lowest of all known eccentric hot Jupiters. WASP-141b (2.7 MJup, 1.2 RJup and P = 3.3 d) and WASP-142b (0.84 MJup, 1.53 RJup and P = 2.1 d) are typical hot Jupiters orbiting metal-rich F stars. We show that the period distribution within the hot-Jupiter bulge does not depend on the metallicity of the host star.
stars: individual: WASP-130 - WASP-131 - WASP-132 - WASP-139 - WASP-140 - WASP-141 - WASP-142 - planetary systems - planetary systems
VizieR on-line data:
<Available at CDS (J/MNRAS/465/3693): stars.dat tablea1.dat>
Status at CDS:
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