Differential rotation of main-sequence dwarfs: predicting the dependence on surface temperature and rotation rate

Gyrochronology and recent theoretical findings are used to reduce the number of input parameters of differential rotation models. This eventually leads, after having fixed our turbulence model parameters, to a theoretical prediction for the surface differential rotation as a function of only two ste...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2012-07, Vol.423 (4), p.3344-3351
Hauptverfasser:	Kitchatinov, L. L., Olemskoy, S. V.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Dwarf stars Mathematical models Stars & galaxies stars: late‐type stars: rotation Turbulent flow
Online-Zugang:	Volltext
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