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.
HD Type $v~\sin{i}$ q₂/q₁ $v_{\rm e, rigid}$ i

[km s^-1] [km s^-1]

89449 F6IV $17.3 \pm 1.7$ 1.44 630 1.7 $^{\circ}$

89569 F6V $12.2 \pm 0.7$ 1.57 500 1.4 $^{\circ}$

100563 F5V $13.5 \pm 0.4$ 1.67 370 2.1 $^{\circ}$

105452 F0IV/V $23.5 \pm 1.2$ 1.59 500 2.7 $^{\circ}$

120136 F7V $15.6 \pm 1.0$ 1.57 500 1.8 $^{\circ}$

121370 G0IV $13.5 \pm 1.3$ 1.46 590 1.3 $^{\circ}$

160915 F6V $12.4 \pm 0.5$ 1.60 470 1.5 $^{\circ}$

173667 F6V $18.0 \pm 2.0$ 1.40 660 1.6 $^{\circ}$

175317 F5IV/V $17.1 \pm 0.7$ 1.58 490 2.0 $^{\circ}$

197692 F5V $41.7 \pm 1.7$ 1.62 440 5.4 $^{\circ}$

**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.
HD	Type	$v~\sin{i}$	q₂/q₁	$v_{\rm e, rigid}$	i
		[km s^-1]		[km s^-1]
89449	F6IV	$17.3 \pm 1.7$	1.44	630	1.7 $^{\circ}$
89569	F6V	$12.2 \pm 0.7$	1.57	500	1.4 $^{\circ}$
100563	F5V	$13.5 \pm 0.4$	1.67	370	2.1 $^{\circ}$
105452	F0IV/V	$23.5 \pm 1.2$	1.59	500	2.7 $^{\circ}$
120136	F7V	$15.6 \pm 1.0$	1.57	500	1.8 $^{\circ}$
121370	G0IV	$13.5 \pm 1.3$	1.46	590	1.3 $^{\circ}$
160915	F6V	$12.4 \pm 0.5$	1.60	470	1.5 $^{\circ}$
173667	F6V	$18.0 \pm 2.0$	1.40	660	1.6 $^{\circ}$
175317	F5IV/V	$17.1 \pm 0.7$	1.58	490	2.0 $^{\circ}$
197692	F5V	$41.7 \pm 1.7$	1.62	440	5.4 $^{\circ}$

Source LaTeX | All tables | In the text