**Table 5:** Data for stars in the region of Bo 7.
LSS	Sp.Type	V^a	B-V^a	E(B-V)	V₀-M_v	RV
						(LSR)
1131	O7.5V	10.80	0.51	0.83	13.33	+50
1132^b	B3V	10.05	0.37	0.54	9.88	-13
1135	O6.5V((f))	10.88	0.40	0.73	13.95	+55
1137	O9V	11.38	0.49	0.80	13.40	+42
1140	B0III	11.65	0.76	1.05	13.49	+40
1144	O7.5V	11.27	0.64	0.96	13.39	+53
1145^c	WN8	10.78	0.56			var.
1146^d	B1III	11.57	0.50	0.82	13.43	+26
1147^e	B1Ve	11.53	0.58	0.78	13.11	+54

^a From Moffat & Vogt (1975).
^b Foreground star, see also Lundstrom & Stenholm (1984).
^c WR 12 cf. van der Hucht (2001). Spectroscopic binary Niemela (1982).
^d Line widths appear variable. May be an unresolved.
double-lined binary?
^e H Balmer lines H $\beta$ and H $\gamma$ show central emission, see Fig. 1.

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