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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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Hlavní autoři: Cecil M., Flock M., Malygin M. G., Kuiper R., Sudarshan P., Ziampras A., Elbakyan V. G.
Médium: Artigo
Jazyk:Inglês
Vydáno: EDP Sciences 2026-03-01
Edice:Astronomy & Astrophysics
Témata:
accretion, accretion disks
hydrodynamics
opacity
radiative transfer
protoplanetary disks
stars: protostars
On-line přístup:https://www.aanda.org/articles/aa/full_html/2026/03/aa57408-25/aa57408-25.html
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