Modeling the effects of starspots on stellar magnetic cycles

Open Access

Fig. 1.

Differential rotations of solar-mass stars. Panels a and b are the profiles of differential rotation for stars with rotation periods of 25 and 13 days, respectively. Panel c shows the latitudinal distribution of the radius-averaged latitudinal shear $\bar{\nabla Ω_{θ}} (θ)$ $\overline{\nabla\Omega_{\theta}}(\theta)$ for the different rotators studied here. The vertical dashed line denotes 55° latitude.

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