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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 720336.0, MPI für Astronomie / Publikationen_mpia
Stellar diameters and temperatures - VI. High angular resolution measurements of the transiting exoplanet host stars HD 189733 and HD 209458 and implications for models of cool dwarfs
Authors:Boyajian, T.; von Braun, K.; Feiden, G. A.; Huber, D.; Basu, S.; Demarque, P.; Fischer, D. A.; Schaefer, G.; Mann, A. W.; White, T. R.; Maestro, V.; Brewer, J.; Lamell, C. B.; Spada, F.; López-Morales, M.; Ireland, M.; Farrington, C.; van Belle, G. T.; Kane, S. R.; Jones, J.; ten Brummelaar, T. A.; Ciardi, D. R.; McAlister, H. A.; Ridgway, S.; Goldfinger, P. J.; Turner, N. H.; Sturmann, L.
Date of Publication (YYYY-MM-DD):2015
Title of Journal:Monthly Notices of the Royal Astronomical Society
Volume:447
Start Page:846
End Page:857
Audience:Not Specified
Abstract / Description:We present direct radii measurements of the well-known transiting exoplanet host stars HD 189733 and HD 209458 using the CHARA Array interferometer. We find the limb-darkened angular diameters to be θLD = 0.3848 ± 0.0055 and 0.2254 ± 0.0072 mas for HD 189733 and HD 209458, respectively. HD 189733 and HD 209458 are currently the only two transiting exoplanet systems where detection of the respective planetary companion's orbital motion from high-resolution spectroscopy has revealed absolute masses for both star and planet. We use our new measurements together with the orbital information from radial velocity and photometric time series data, Hipparcos distances, and newly measured bolometric fluxes to determine the stellar effective temperatures (Teff = 4875 ± 43, 6092 ± 103 K), stellar linear radii (R* = 0.805 ± 0.016, 1.203 ± 0.061 R), mean stellar densities (ρ* = 1.62 ± 0.11, 0.58 ± 0.14 ρ), planetary radii (Rp = 1.216 ± 0.024, 1.451 ± 0.074 RJup), and mean planetary densities (ρp = 0.605 ± 0.029, 0.196 ± 0.033 ρJup) for HD 189733b and HD 209458b, respectively. The stellar parameters for HD 209458, an F9 dwarf, are consistent with indirect estimates derived from spectroscopic and evolutionary modelling. However, we find that models are unable to reproduce the observational results for the K2 dwarf, HD 189733. We show that, for stellar evolutionary models to match the observed stellar properties of
Free Keywords:techniques: interferometric; stars: fundamental parameters; stars: individual: HD 189733; stars: individual: HD 209458; stars: late-type; infrared: stars
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:ISSN:0035-8711
URL:http://cdsads.u-strasbg.fr/abs/2015MNRAS.447..846B
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