Kinematic Evidence of an Embedded Protoplanet in HD 142666 Identified by Machine Learning

Kinematic Evidence of an Embedded Protoplanet in HD 142666 Identified by Machine Learning

Observations of protoplanetary disks have shown that forming exoplanets leave characteristic imprints on the gas and dust of the disk. In the gas, these forming exoplanets cause deviations from Keplerian motion, which can be detected through molecular line observations. Our previous work has shown t...

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Bibliographic Details
Main Authors: J. P. Terry, C. Hall, S. Abreau, S. Gleyzer
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Protoplanetary disks
Planetary system formation
Hydrodynamical simulations
Astronomical simulations
Radiative transfer simulations
Online Access:https://doi.org/10.3847/1538-4357/acc737

Internet

https://doi.org/10.3847/1538-4357/acc737

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