76 citations · 361 across the 6 of their papers we have counts for
6 papers
Disk-Planet Interaction Simulations: (I) Baroclinic Generation of Vortensity and Non-Axisymmetric Rossby-Wave-Instability
Shangli Ou, Jianghui Ji, Lin Liu +1
We use a multi-dimensional hydrodynamics code to study the gravitational interaction between an embedded planet and a protoplanetary disk with emphasis on the generation of vortens…
The Secular Evolution and Dynamical Architecture of the Neptunian Triplet Planetary System HD 69830
Ji Jianghui, H. Kinoshita, Liu Lin +1
We perform numerical simulations to study the secular orbital evolution and dynamical structure in the HD 69830 system with the best-fit orbital solutions by Lovis and coworkers (2…
Could the 47 UMa Planetary System be a Second Solar System: predicting the Earth-like planets
Jianghui Ji, Lin Liu, H. Kinoshita +1
(Abridged)We numerically investigated the dynamical architecture of 47 UMa with the planetary configuration of the best-fit orbital solutions by Fischer et al. We systematically st…
The Librating Companions in HD 37124, HD 12661, HD 82943, 47 Uma and GJ 876: Alignment or Antialignment?
Jianghui Ji, Lin Liu, H. Kinoshita +3
We investigated the apsidal motion for the multi-planet systems. In the simulations, we found that the two planets of HD 37124, HD 12661, 47 Uma and HD 82943 separately undergo aps…
The Apsidal Antialignment of the HD 82943 System
Ji Jianghui, H. Kinoshita, Liu Lin +2
We perform numerical simulations to explore the dynamical evolution of the HD 82943 planetary system. By simulating diverse planetary configurations, we find two mechanisms of stab…
Could the 55 Cancri Planetary System Really Be in the 3:1 Mean Motion Resonance?
Ji Jianghui, H. Kinoshita, Liu Lin +1
We integrate the orbital solutions of the planets orbiting 55 Cnc. In the simulations, we find that not only three resonant arguments , $θ_{2}=λ_{1…