Electronic Resource

Validation of the exoplanet Kepler-21b using PAVO/CHARA long-baseline interferometry

التفاصيل البيبلوغرافية
العنوان: Validation of the exoplanet Kepler-21b using PAVO/CHARA long-baseline interferometry
المؤلفون: Huber, D, Ireland, Michael, Bedding, Timothy Russell, Howell, Steve B, Maestro, V, Merand, A, Tuthill, Peter G, White, T. R, Farrington, C, Goldfinger, P. J, McAlister, H, Schaefer, G. H, Sturmann, J, Sturmann, Laszlo, ten Brummelaar, Theo, Turner, Nils
المصدر: Monthly Notices of the Royal Astronomical Society: Letters
بيانات النشر: Blackwell Publishing 2012
نوع الوثيقة: Electronic Resource
مستخلص: We present long-baseline interferometry of the Kepler exoplanet host star HD179070 (Kepler-21) using the Precision Astronomical Visible Observations (PAVO) beam combiner at the Center for High Angular Resolution Astronomy (CHARA) Array. The visibility data are consistent with a single star and exclude stellar companions at separations ~1-1000 mas (~0.1-113 au) and contrasts <3.5 mag. This result supports the validation of the 1.6R⊕ exoplanet Kepler-21b by Howell et al. and complements the constraints set by adaptive optics imaging, speckle interferometry and radial-velocity observations to rule out false positives due to stellar companions. We conclude that long-baseline interferometry has strong potential to validate transiting extrasolar planets, particularly for future projects aimed at brighter stars and for host stars where radial-velocity follow-up is not available.
مصطلحات الفهرس: Keywords: Planets and satellites: individual: Kepler-2lb; Stars: individual: HD 179070; Techniques: interferometric, Journal article
URL: http://hdl.handle.net/1885/66577
الاتاحة: Open access content. Open access content
Author/s retain copyright
Other Numbers: AUANP oai:openresearch-repository.anu.edu.au:1885/66577
1745-3933
1291793016
المصدر المساهم: AUSTRALIAN NAT UNIV - PRINT REPOSITORY
From OAIster®, provided by the OCLC Cooperative.
رقم الانضمام: edsoai.on1291793016
قاعدة البيانات: OAIster