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Shear-driven transport and mixing in the interiors of massive stars
Published online by Cambridge University Press: 28 July 2017
Abstract
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Turbulent transport and mixing generated by hydrodynamic instabilities triggered by rotation gradients are key mechanisms in the evolution of massive stars. We present here a summary of the progresses on shear-induced mixing obtained with numerical simulations, along with a new prescription for horizontal turbulence.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 12 , Symposium S329: The Lives and Death-Throes of Massive Stars , November 2016 , pp. 434
- Copyright
- Copyright © International Astronomical Union 2017
References
Mathis, S., Amard, L., Charbonnel, C., Palacios, A., & Prat, V., 2017a, A&A, submittedGoogle Scholar
Mathis, S., Prat, V., Amard, L., Charbonnel, C., & Palacios, A., 2017b, A&A, submittedGoogle Scholar