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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| Главные авторы: | , , |
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| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
EDP Sciences
2026-01-01
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| Серии: | Astronomy & Astrophysics |
| Предметы: | |
| Online-ссылка: | https://www.aanda.org/articles/aa/full_html/2026/01/aa56316-25/aa56316-25.html |
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