Resonant Chains and the Convergent Migration of Planets in Protoplanetary Disks
An increasing number of compact planetary systems with multiple planets in a resonant chain have been detected. The resonant chain must be maintained by convergent migration of the planets due to planet–disk interactions if it is formed before the dispersal of the protoplanetary gas disk. For type I...
Main Authors: | Ka Ho Wong, Man Hoi Lee |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2024-01-01
|
Series: | The Astronomical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-3881/ad1f60 |
Similar Items
-
The Dependence of the Structure of Planet-opened Gaps in Protoplanetary Disks on Radiative Cooling
by: Minghao Zhang, et al.
Published: (2024-01-01) -
Resonant Excitation of Planetary Eccentricity due to a Dispersing Eccentric Protoplanetary Disk: A New Mechanism of Generating Large Planetary Eccentricities
by: Jiaru Li, et al.
Published: (2023-01-01) -
Dust Drift Timescales in Protoplanetary Disks at the Cusp of Gravitational Instability
by: Jonathan P. Williams, et al.
Published: (2024-01-01) -
Long-term Protoplanetary Disk Evolution from Molecular Cloud Core Collapse and Implications for Planet Formation. I. Weak and Moderate Disk Self-gravities
by: Xin-Ming Wang
Published: (2023-01-01) -
Streaming Torque in Dust–Gas Coupled Protoplanetary Disks
by: Qiang Hou, et al.
Published: (2024-01-01)