Dust Dynamics in Radially Convective Regions of Protoplanetary Disks
Hydrodynamic instabilities likely operate in protoplanetary disks. One candidate, convective overstability (COS), can be triggered in regions with a negative radial entropy gradient. The ensuing turbulence and flow structures are expected to affect dust dynamics directly. We revisit the interaction...
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| Principais autores: | , |
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| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
IOP Publishing
2025-01-01
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| Serija: | The Astrophysical Journal |
| Teme: | |
| Online dostop: | https://doi.org/10.3847/1538-4357/adabe6 |
| Oznake: |
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