Long-term Stability of Planetary Systems Formed from a Transitional Disk

Transitional disks are protoplanetary disks with large and deep central holes in the gas, possibly carved by young planets. Dong & Dawson simulated systems with multiple giant planets that were capable of carving and maintaining such gaps during the disk stage. Here we continue their simulations...

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Bibliographic Details
Main Authors: Rory Bowens, Andrew Shannon, Rebekah Dawson, Jiayin Dong
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/acb13c