One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c

2015/03/31 by David J. Armstrong, D. J. Armstrong, Alexandre Santerne +48 · 48 citations
Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Exoplanet #Mean motion #Neptune #Particle physics #Photometry (optics) #Physics #Planet #Proper motion #Resonance (particle physics) #Stars #Stellar, planetary, and galactic studies #Telescope #Transit (satellite) #astro-ph.EP

paper · pdf · doi:10.1051/0004-6361/201526008

published in Astronomy and Astrophysics 582, A33 (EDP Sciences) · 18 pages, 10 figures, accepted to A&A, updated to match published version

openalex publication_date 2015/08/24 · arxiv created 2015/09/02 · arxiv updated 2015/10/07 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. The K2 mission has recently begun to discover new and diverse planetary systems. In December 2014, Campaign 1 data from the mission was released, providing high-precision photometry for ~22 000 objects over an 80-day timespan. We searched these data with the aim of detecting more important new objects.

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Cited by

• Mass determination of K2-19b and K2-19c from radial velocities and transit timing variations