XUE: Thermochemical Modeling Suggests a Compact and Gas-depleted Structure for a Distant, Irradiated Protoplanetary Disk

XUE: Thermochemical Modeling Suggests a Compact and Gas-depleted Structure for a Distant, Irradiated Protoplanetary Disk

Unveiling the physical structure of protoplanetary disks is crucial for interpreting the diversity of the exoplanet population. Until recently, the census of the physical properties of protoplanetary disks probed by mid-infrared observations was limited to the solar neighborhood ( d  ≲ 250 pc). Howe...

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Bibliographic Details
Main Authors: Bayron Portilla-Revelo, Konstantin V. Getman, María Claudia Ramírez-Tannus, Thomas J. Haworth, Rens Waters, Arjan Bik, Eric D. Feigelson, Inga Kamp, Sierk E. van Terwisga, Jenny Frediani, Thomas Henning, Andrew J. Winter, Veronica Roccatagliata, Thomas Preibisch, E. Sabbi, Peter Zeidler, Michael A. Kuhn
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Star forming regions
Planet formation
Protoplanetary disks
Infrared spectroscopy
Radiative transfer simulations
Online Access:https://doi.org/10.3847/1538-4357/adc91d
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https://doi.org/10.3847/1538-4357/adc91d

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