All Tables

Table 1: Parameters of the calculated models, a and b are parameters used in Eq. (4) with values of gravity darkening $\beta$ according to Claret (1998). Note that for all models profiles with $\beta = 0.0, 0.08$ and 0.25 were analyzed.
Table 2: Stars with measured values q₂/q₁ < 1.72 from the sample of Reiners & Schmitt (2003); differential rotation is claimed for these objects. Interpreting the values of q₂/q₁ as due to very fast rotation seen under small inclination angles, the required values of $v_{\rm e, rigid}$ and i are given. Nine of the ten are larger than break-up velocity.