Inferring the physics of protoplanetary disc evolution from the irradiated Cygnus OB2 region

Context. Determining the physical processes driving protoplanetary disc evolution is of paramount importance for understanding planet formation. Our current understanding has crystallised around two possible evolution scenarios: turbulent viscosity and magnetohydrodynamic (MHD) wind-driven. Which of...

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Principais autores:	Weder Jesse, Winter Andrew J., Mordasini Christoph
Formato:	Artigo
Idioma:	Inglês
Publicado em:	EDP Sciences 2026-01-01
coleção:	Astronomy & Astrophysics
Assuntos:	accretion, accretion disks magnetohydrodynamics (mhd) turbulence protoplanetary disks
Acesso em linha:	https://www.aanda.org/articles/aa/full_html/2026/01/aa56316-25/aa56316-25.html
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