On turbulence driven by axial precession and tidal evolution of the spin–orbit angle of close-in giant planets
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/460/3/2339/8130166/stw1172.pdf
Reference60 articles.
1. Misaligned spin and orbital axes cause the anomalous precession of DI Herculis
2. THE BANANA PROJECT. V. MISALIGNED AND PRECESSING STELLAR ROTATION AXES IN CV VELORUM
3. Non-linear tides in a homogeneous rotating planet or star: global simulations of the elliptical instability
4. Non-linear evolution of the tidal elliptical instability in gaseous planets and stars
5. Non-linear evolution of the elliptical instability in the presence of weak magnetic fields
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