Table 6: The mean projected rotational velocities for our higher gravity targets ( $\log~g \geq 3.9$ ; designated "High gravity'') and our apparently evolved targets excluding known supergiants ( $\log~g < 3.9$ ; designated "Low gravity''). The number of stars in each sample is given by n.
Cluster High gravity n Low gravity n

$\mbox{km~s}^{-1}$ $\mbox{km~s}^{-1}$

NGC 3293 $184\pm99$ 47 $196\pm95$ 41

NGC 4755 $173\pm71$ 47 $211\pm96$ 38

NGC 6611 $132\pm75$ 22 $187\pm73$ 6

All targets $170\pm86$ 116 $202\pm94$ 85

**Table 6:** The mean projected rotational velocities for our higher gravity targets ( $\log~g \geq 3.9$ ; designated "High gravity'') and our apparently evolved targets excluding known supergiants ( $\log~g < 3.9$ ; designated "Low gravity''). The number of stars in each sample is given by n.
Cluster	High gravity	n	Low gravity	n
	$\mbox{km~s}^{-1}$	$\mbox{km~s}^{-1}$
NGC 3293	$184\pm99$	47	$196\pm95$	41
NGC 4755	$173\pm71$	47	$211\pm96$	38
NGC 6611	$132\pm75$	22	$187\pm73$	6

All targets	$170\pm86$	116	$202\pm94$	85

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