Fig. 18
Projected rotational velocity normalized to critical velocity, νesini/ vcrit, vs. spectral subtype for our sample stars with known spectral types. Critical velocities are estimated using the SpT calibration by Weidner & Vink (2010). See legend for the information on the luminosity class. Stars indicated in the legend as “upper limits” refer to stars with νesini ≤ 40 kms-1.
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