The Effect of Ultraviolet Photon Pumping of H2 in Dust-deficient Protoplanetary Disks

We perform radiation hydrodynamics simulations to study the structure and evolution of a photoevaporating protoplanetary disk. Ultraviolet and X-ray radiation from the host star heats the disk surface, where H _2 pumping also operates efficiently. We run a set of simulations in which we varied the n...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	Ayano Komaki, Rolf Kuiper, Naoki Yoshida
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Protoplanetary disks Planet formation Hydrodynamical simulations Star formation Interstellar medium
Online Access:	https://doi.org/10.3847/1538-4357/ad21f1