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Vertical Shear Instability in the Solar Nebula
Published online by Cambridge University Press: 27 January 2016
Abstract
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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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 10 , Issue S314: Young Stars & Planets Near the Sun , November 2015 , pp. 195 - 196
- Copyright
- Copyright © International Astronomical Union 2016
References
Chiang, E. & Youdin, A. N. 2010, Annual Review of Earth and Planetary Sciences, 38, 493CrossRefGoogle Scholar
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