126 citations · 383 across the 7 of their papers we have counts for
7 papers
Turbulent infall onto class 0 disks as cause of CAI brief condensation episode in the solar system
Jiachen Zheng, Xing Wei, Hongping Deng +2
Calcium-aluminum-rich inclusions (CAIs) in carbonaceous chondritic meteorites are the oldest relics in the solar system. Notably, their radiogenic age feature a brief (100 kyr) con…
Chaotic migration of LISA Extreme Mass Ratio Inspirals in a turbulent accretion disk: effect on waveform de-phasing
Mudit Garg, Lucio Mayer, Yinhao Wu +2
Gravitational wave (GW) detector LISA will observe near-coalescence extreme mass ratio inspirals (EMRIs), which typically form in galactic central accretion disks. Torques from the…
Embryo impacts and gas giant mergers II: Diversity of Hot Jupiters' internal structure
Shang-Fei Liu, Craig B. Agnor, D. N. C. Lin +1
We consider the origin of compact, short-period, Jupiter-mass planets. We propose that their diverse structure is caused by giant impacts of embryos and super-Earths or mergers wit…
On the Migration of Jupiter and Saturn: Constraints from Linear Models of Secular Resonant Coupling with the Terrestrial Planets
Craig B. Agnor, D. N. C. Lin
We examine how the late divergent migration of Jupiter and Saturn may have perturbed the terrestrial planets. We identify six secular resonances between the nu_5 apsidal eigenfrequ…
Embryo impacts and gas giant mergers I: Dichotomy of Jupiter and Saturn's core mass
Shu Lin Li, C. B. Agnor, D. N. C. Lin
Interior to the gaseous envelopes of Saturn, Uranus, and Neptune, there are high-density cores with masses larger than 10 Earth masses. According to the conventional sequential acc…
Type I planet migration in nearly laminar disks - long term behavior
Cong Yu, Hui Li, Shengtai Li +2
We carry out 2-D high resolution numerical simulations of type I planet migration with different disk viscosities. We find that the planet migration is strongly dependent on disk v…
Type I Planet Migration in Nearly Laminar Disks
H. Li, S. H. Lubow, S. Li +1
We describe 2D hydrodynamic simulations of the migration of low-mass planets () in nearly laminar disks (viscosity parameter ) over timescales of se…