The Time Evolution of in Protoplanetary Disks as a Way to Disentangle between Viscosity and MHD Winds
As the classic viscous paradigm for protoplanetary disk accretion is challenged by the observational evidence of low turbulence, the alternative scenario of MHD disk winds is being explored as being potentially able to reproduce the same observed features traditionally explained with viscosity. Alth...
Gardado en:
| Principais autores: | , , , , , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
IOP Publishing
2023-01-01
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| Series: | The Astrophysical Journal Letters |
| Assuntos: | |
| Acceso en liña: | https://doi.org/10.3847/2041-8213/acf048 |
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