The Inner Disk Rim of HD 163296: Linking Radiative Hydrostatic Models with Infrared Interferometry

The Inner Disk Rim of HD 163296: Linking Radiative Hydrostatic Models with Infrared Interferometry

Previous studies of the protoplanetary disk HD 163296 revealed that the morphology of its sub-au infrared emission encompasses the terminal sublimation front of dust grains, referred to as the inner rim, but also extends into the (supposedly) dust-free region within it. Here, we present a set of rad...

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Bibliographic Details
Main Authors: Ondřej Chrenko, Mario Flock, Takahiro Ueda, Antoine Mérand, Myriam Benisty, Raúl O. Chametla
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astronomical Journal
Subjects:
Protoplanetary disks
Planet formation
Radiative transfer
Interferometry
Exoplanets
Online Access:https://doi.org/10.3847/1538-3881/ad234d

Internet

https://doi.org/10.3847/1538-3881/ad234d

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