Fig. 7.
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Flaring activity vs. inclination for stars in the unsaturated regime. In order to reduce the influence of rotation, the Rossby number was divided into three intervals. The large uncertainty is due to the decline in v sin i with decreasing rotation and our conservative policy for stars of v sin i < 10 km s−1 (their upper limit and lower limit were set to be 1 km s−1 and 10 km s−1, respectively).
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