Table 5: Heliocentric radial velocity (with its standard error) of the program stars, binary status and cluster membership according to radial velocities, and projected rotational velocity (with its standard error). The radial velocity of the binary stars is the barycentric velocity from the orbital solutions in Table 6. The last column gives the projected rotation period / of the solved binaries to be compared with the orbital period.

#		binary	member		/
	(km s-1)			(km s-1)	(days)
1		yes	no		5.0
2		yes	yes		10
3		yes	yes		15
4		yes	yes		10
5		no	yes
6		yes	(yes)
7		yes	yes		3.8
8		no	yes
9		no	no
10		no	yes
11		yes	no		11
12		yes	yes		1.5
13		no	yes
14		no	yes
15		no	yes
16		yes	(yes)