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XUE. Modeling MIR Molecular Gas Tracers of Truncation in Highly Irradiated Planet-forming Disks

High-mass star-forming regions (SFRs), dominated by intense far-ultraviolet (FUV) radiation fields (∼10 ^5 G _0 ) from nearby O stars, are the birthplaces of most planetary systems. While our understanding of protoplanetary disks (PPDs) and their evolution has primarily come from observations of iso...

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Autors principals: Sebastian Hernández Arboleda, Germán Chaparro, Pablo Cuartas-Restrepo, Inga Kamp, María Claudia Ramírez-Tannus, Arjan Bik, Jenny Frediani, Thomas Haworth, Thomas Henning, Michael A. Kuhn, Thomas Preibisch, Bayron Portilla-Revelo, Elena Sabbi, Veronica Roccatagliata, Sierk E. van Terwisga, Andrew Winter
Format: Artigo
Idioma:Inglês
Publicat: IOP Publishing 2026-01-01
Col·lecció:The Astrophysical Journal
Matèries:
Protoplanetary disks
Pre-main sequence stars
Proplyds
Polycyclic aromatic hydrocarbons
Radiative transfer simulations
Accés en línia:https://doi.org/10.3847/1538-4357/ae5b83
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