Evolution of a protoplanetary disc with the magnetic wind
Theoretical studies and numerical simulations of the protoplanetary discs (PPDs) indicate that magnetorotational instability (MRI) is a dominant mechanism in the accretion process. Recent observational evidence, however, implies that magnetic winds present in these systems. Launching the magnetic wi...
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| Format: | Article |
| Language: | English |
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Isfahan University of Technology
2020-11-01
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| Series: | Iranian Journal of Physics Research |
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| Online Access: | http://ijpr.iut.ac.ir/article_1641_002882e682181a4f5ad532b527187eb4.pdf |