Based on the model described in , we present an analytical+numerical study of the resonance capture under Type-I migration for the Kepler-25  and K2-24  Kepler systems, both close to a 2/1 mean-motion resonance. We find that, depending on the flare index and the proximity to the central star, the average value of the period-ratio between two consecutive planets show a significant deviation with respect to the resonant nominal value, up to values well in agreement with the observations.
|Journal||Journal of Physics: Conference Series|
|State||Published - 25 Oct 2017|
|Event||18th Brazilian Colloquium on Orbital Dynamics, CBDO 2016 - Aguas de Lindoia, Brazil|
Duration: 28 Nov 2016 → 2 Dec 2016