SIMBAD references

2016AJ....151...89B - Astron. J., 151, 89 (2016/April-0)

HATS-17b: a transiting compact warm Jupiter in a 16.3 day circular orbit.

BRAHM R., JORDAN A., BAKOS G.A., PENEV K., ESPINOZA N., RABUS M., HARTMAN J.D., BAYLISS D., CICERI S., ZHOU G., MANCINI L., TAN T.G., DE VAL-BORRO M., BHATTI W., CSUBRY Z., BENTO J., HENNING T., SCHMIDT B., ROJAS F., SUC V., LAZAR J., PAPP I. and SARI P.

Abstract (from CDS):

We report the discovery of HATS-17b, the first transiting warm Jupiter of the HATSouth network. HATS-17b transits its bright (V = 12.4) G-type (M* = 1.131 ± 0.030 M, R* = 1.090–0.046+0.070) metal-rich ([Fe/H] = +0.3 dex) host star in a circular orbit with a period of P = 16.2546 days. HATS-17b has a very compact radius of 0.777± 0.056 RJ given its Jupiter-like mass of 1.338 ± 0.065 MJ. Up to 50% of the mass of HATS-17b may be composed of heavy elements in order to explain its high density with current models of planetary structure. HATS-17b is the longest period transiting planet discovered to date by a ground-based photometric survey, and is one of the brightest transiting warm Jupiter systems known. The brightness of HATS-17 will allow detailed follow-up observations to characterize the orbital geometry of the system and the atmosphere of the planet.

Abstract Copyright:

Journal keyword(s): planetary systems - stars: individual: HATS-17 - techniques: photometric - techniques: spectroscopic

VizieR on-line data: <Available at CDS (J/AJ/151/89): table2.dat table3.dat>

Simbad objects: 12

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2022.09.30-15:28:00

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