TY - JOUR
T1 - Orbital migration and Resonance Offset of the Kepler-25 and K2-24 systems
AU - Charalambous, C.
AU - Ramos, X. S.
AU - Benitez-Llambay, P.
AU - Beaugé, C.
N1 - Publisher Copyright:
© Published under licence by IOP Publishing Ltd.
PY - 2017/10/25
Y1 - 2017/10/25
N2 - Based on the model described in [1], we present an analytical+numerical study of the resonance capture under Type-I migration for the Kepler-25 [2] and K2-24 [3] 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.
AB - Based on the model described in [1], we present an analytical+numerical study of the resonance capture under Type-I migration for the Kepler-25 [2] and K2-24 [3] 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.
UR - http://www.scopus.com/inward/record.url?scp=85034636703&partnerID=8YFLogxK
U2 - 10.1088/1742-6596/911/1/012027
DO - 10.1088/1742-6596/911/1/012027
M3 - Conference article
AN - SCOPUS:85034636703
SN - 1742-6588
VL - 911
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
IS - 1
M1 - 012027
T2 - 18th Brazilian Colloquium on Orbital Dynamics, CBDO 2016
Y2 - 28 November 2016 through 2 December 2016
ER -