Timescale diagnostics for saving viscous and MHD-wind-driven dusty discs from external photoevaporation
Context. The evolution of protoplanetary discs is a function of their internal processes and of the environment in which the discs are located. It is unclear if angular momentum is mainly removed viscously or by magnetic winds or by a combination of the two. While external photoevaporation is expect...
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| Hoofdauteurs: | , , , |
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| Formaat: | Artigo |
| Taal: | Inglês |
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EDP Sciences
2026-03-01
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| Reeks: | Astronomy & Astrophysics |
| Onderwerpen: | |
| Online toegang: | https://www.aanda.org/articles/aa/full_html/2026/03/aa58535-25/aa58535-25.html |
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