HATS9-b and HATS10-b: TWO COMPACT HOT JUPITERS in FIELD 7 of the K2 MISSION

  • R. Brahm
  • , A. Jordán
  • , J. D. Hartman
  • , G. Bakos
  • , D. Bayliss
  • , K. Penev
  • , G. Zhou
  • , S. Ciceri
  • , M. Rabus
  • , N. Espinoza
  • , L. Mancini
  • , M. De Val-Borro
  • , W. Bhatti
  • , B. Sato
  • , T. G. Tan
  • , Z. Csubry
  • , L. Buchhave
  • , T. Henning
  • , B. Schmidt
  • , V. Suc
  • R. W. Noyes, I. Papp, J. Lázár, P. Sári

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

32 Citas (Scopus)

Resumen

We report the discovery of two transiting extrasolar planets by the HATSouth survey. HATS-9b orbits an old (10.8 ± 1.5 Gyr) V = 13.3 G dwarf star with a period days. The host star has a mass of 1.03 M⊙, radius of 1.503 R⊙, and effective temperature 5366 ± 70 K. The planetary companion has a mass of 0.837 Mj and radius of 1.065 Rj, yielding a mean density of 0.85g cm-3. HATS-10b orbits a V = 13.1 G dwarf star with a period days. The host star has a mass of 1.1 M⊙, radius of 1.11 R⊙, and effective temperature 5880 ± 120 K. The planetary companion has a mass of 0.53 and radius of 0.97 , yielding a mean density of 0.7 g cm-3. Both planets are compact in comparison with planets receiving similar irradiation from their host stars and lie in the nominal coordinates of Field 7 of K2, but only HATS-9b falls on working silicon. Future characterization of HATS-9b with the exquisite photometric precision of the Kepler telescope may provide measurements of its reflected light signature.

Idioma originalInglés
Número de artículo33
PublicaciónAstronomical Journal
Volumen150
N.º1
DOI
EstadoPublicada - 1 jul. 2015
Publicado de forma externa

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