The role of detailed gas and dust opacities in shaping the evolution of the inner disc edge subject to episodic accretion

Context. The transition in turbulence in the inner regions of protoplanetary discs and the closely connected dust sublimation front lead to a periodic instability, manifesting as episodic accretion outbursts. For the corresponding interplay between heating and cooling, the opacity of the material ne...

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Autors principals:	Cecil M., Flock M., Malygin M. G., Kuiper R., Sudarshan P., Ziampras A., Elbakyan V. G.
Format:	Artigo
Idioma:	Inglês
Publicat:	EDP Sciences 2026-03-01
Col·lecció:	Astronomy & Astrophysics
Matèries:	accretion, accretion disks hydrodynamics opacity radiative transfer protoplanetary disks stars: protostars
Accés en línia:	https://www.aanda.org/articles/aa/full_html/2026/03/aa57408-25/aa57408-25.html
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