Abstract
We quantify the thermodynamic requirement for the Vertical Shear Instability and evaluate its relevance to realistic protoplanetary disks as a potential route to hydrodynamic turbulence.
Original language | English (US) |
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Pages (from-to) | 195-196 |
Number of pages | 2 |
Journal | Proceedings of the International Astronomical Union |
Volume | 10 |
DOIs | |
State | Published - 2015 |
Keywords
- accretion
- accretion disks
- hydrodynamics
- instabilities
- methods: analytical
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science