Table 1: Parameters of the program stars. The data were taken from the Bright Star Catalogue (Hoffleit & Warren 1991). Distances have been calculated using HIPPARCOS parallaxes (ESA 1997). The last column indicates whether a star was observed from ESO (E) or SAO (S).
HR Name HD m_v Sp. $T_{\rm eff}$ $\log g$ $v \sin i$ d RA DEC Obs.

Type (K) $(\mbox{cm~s}^{-2}$ ) (km s^-1) (pc) h m s $^{\circ}$ $^{\prime}$ $^{\prime}$ $^{\prime}$

806 $\epsilon$ Hyi 16 978 4.11 B9 V 10 910 4.29 $100\pm2$ 47.01 02 39 35 - 68 16 01 E

1070 17 Eri 21 790 4.73 B9 V 11 540 3.61 $86\pm2$ 116.69 03 30 37 - 05 04 31 E

1092 22 252 5.83 B8 V 11 860 3.27 $260\pm15$ 261.10 03 30 52 - 66 29 23 E

1214 24 626 5.11 B6 V 14 300 4.12 $29\pm2$ 108.81 03 53 39 - 34 43 56 E

1339 53 Tau 27 295 5.35 B9 IV 12 000 4.19 $5\pm2$ 81.96 04 19 26 + 21 08 32 S

1582 62 Eri 31 512 5.51 B6 V 15 190 3.87 $89\pm4$ 226.76 04 56 24 - 05 10 17 E

1723 34 310 5.07 B9 V 11 180 4.12 $158\pm2$ 83.47 05 15 24 - 26 56 36 E

1728 17 Aur 34 364 6.14 B9.5 V 11 010 4.34 $30\pm4$ 121.95 05 18 19 + 33 46 02 S

1973 38 170 5.29 B9.5 V 10 250 3.69 $60\pm4$ 111.24 05 42 15 - 34 40 04 E

2056 $\lambda$ Col 39 764 4.87 B5 V 15 370 4.22 $101\pm3$ 104.71 05 53 07 - 33 48 05 E

2948 61 555 4.50 B6 V 15 460 4.20 $50\pm5$ 139.28 07 38 49 - 26 48 06 E

3158 66 552 6.15 B9 V 10 450 4.09 $75\pm4$ 91.57 08 04 45 + 18 50 32 S

3439 74 067 5.20 B9 V 10 880 4.14 $36\pm3$ 85.98 08 40 19 - 40 51 15 E

3717 80 781 6.28 B5 V 14 980 3.22 $30\pm3$ 1052.63 09 19 33 - 55 11 12 E

4116 $\delta$ Sex 90 882 5.21 B9.5 V 10 360 3.84 $140\pm3$ 91.99 10 29 29 - 02 44 21 S

4119 $\beta$ Sex 90 994 5.09 B6 V 14 570 4.21 $85\pm4$ 105.71 10 30 18 - 00 38 13 E

4943 14 CVn 113 797 5.25 B9 V 11 260 4.06 $130\pm3$ 86.58 13 05 45 + 35 47 56 S

5501 108 Vir 129 956 5.69 B9.5 V 10 250 3.75 $84\pm4$ 188.32 14 45 30 + 00 43 02 E

5685 $\beta$ Lib 135 742 2.61 B8 V 12 040 3.26 $320\pm20$ 49.06 15 17 00 - 09 22 59 S

5994 $\iota^{2}$ Nor 144 480 5.57 B9.5 V 10 580 4.29 $87\pm3$ 83.19 16 09 19 - 57 56 04 E

6628 161 840 4.83 B8 V 11 990 3.38 $38\pm2$ 186.22 17 49 11 - 31 42 12 E

6633 161 941 6.22 B9.5 V 9960 3.26 $36\pm3$ 757.58 17 48 20 + 03 48 15 E

6647 162 374 5.90 B6 V 16 900 3.72 $38\pm2$ 254.45 17 52 14 - 34 47 57 E

6668 162 817 5.96 B9.5 V 9190 3.15 $76\pm4$ 258.40 17 54 27 - 34 27 59 E

6878 169 009 6.33 B9.5 V 10 440 3.95 $47\pm5$ 105.15 18 23 02 - 10 13 07 E

7337 $\beta^{1}$ Sgr 181 454 4.01 B9 V 11 960 3.83 $77\pm2$ 116.01 19 22 38 - 44 27 32 E

8781 $\alpha$ Peg 218 045 2.49 B9 V 9810 3.51 $130\pm2$ 42.80 23 04 46 + 15 12 19 S

**Table 1:** Parameters of the program stars. The data were taken from the Bright Star Catalogue (Hoffleit & Warren 1991). Distances have been calculated using HIPPARCOS parallaxes (ESA 1997). The last column indicates whether a star was observed from ESO (E) or SAO (S).
HR	Name	HD	m_v	Sp.	$T_{\rm eff}$	$\log g$	$v \sin i$	d	RA	DEC	Obs.
				Type	(K)	$(\mbox{cm~s}^{-2}$ )	(km s^-1)	(pc)	h m s	$^{\circ}$ $^{\prime}$ $^{\prime}$ $^{\prime}$
806	$\epsilon$ Hyi	16 978	4.11	B9 V	10 910	4.29	$100\pm2$	47.01	02 39 35	- 68 16 01	E
1070	17 Eri	21 790	4.73	B9 V	11 540	3.61	$86\pm2$	116.69	03 30 37	- 05 04 31	E
1092		22 252	5.83	B8 V	11 860	3.27	$260\pm15$	261.10	03 30 52	- 66 29 23	E
1214		24 626	5.11	B6 V	14 300	4.12	$29\pm2$	108.81	03 53 39	- 34 43 56	E
1339	53 Tau	27 295	5.35	B9 IV	12 000	4.19	$5\pm2$	81.96	04 19 26	+ 21 08 32	S
1582	62 Eri	31 512	5.51	B6 V	15 190	3.87	$89\pm4$	226.76	04 56 24	- 05 10 17	E
1723		34 310	5.07	B9 V	11 180	4.12	$158\pm2$	83.47	05 15 24	- 26 56 36	E
1728	17 Aur	34 364	6.14	B9.5 V	11 010	4.34	$30\pm4$	121.95	05 18 19	+ 33 46 02	S
1973		38 170	5.29	B9.5 V	10 250	3.69	$60\pm4$	111.24	05 42 15	- 34 40 04	E
2056	$\lambda$ Col	39 764	4.87	B5 V	15 370	4.22	$101\pm3$	104.71	05 53 07	- 33 48 05	E
2948		61 555	4.50	B6 V	15 460	4.20	$50\pm5$	139.28	07 38 49	- 26 48 06	E
3158		66 552	6.15	B9 V	10 450	4.09	$75\pm4$	91.57	08 04 45	+ 18 50 32	S
3439		74 067	5.20	B9 V	10 880	4.14	$36\pm3$	85.98	08 40 19	- 40 51 15	E
3717		80 781	6.28	B5 V	14 980	3.22	$30\pm3$	1052.63	09 19 33	- 55 11 12	E
4116	$\delta$ Sex	90 882	5.21	B9.5 V	10 360	3.84	$140\pm3$	91.99	10 29 29	- 02 44 21	S
4119	$\beta$ Sex	90 994	5.09	B6 V	14 570	4.21	$85\pm4$	105.71	10 30 18	- 00 38 13	E
4943	14 CVn	113 797	5.25	B9 V	11 260	4.06	$130\pm3$	86.58	13 05 45	+ 35 47 56	S
5501	108 Vir	129 956	5.69	B9.5 V	10 250	3.75	$84\pm4$	188.32	14 45 30	+ 00 43 02	E
5685	$\beta$ Lib	135 742	2.61	B8 V	12 040	3.26	$320\pm20$	49.06	15 17 00	- 09 22 59	S
5994	$\iota^{2}$ Nor	144 480	5.57	B9.5 V	10 580	4.29	$87\pm3$	83.19	16 09 19	- 57 56 04	E
6628		161 840	4.83	B8 V	11 990	3.38	$38\pm2$	186.22	17 49 11	- 31 42 12	E
6633		161 941	6.22	B9.5 V	9960	3.26	$36\pm3$	757.58	17 48 20	+ 03 48 15	E
6647		162 374	5.90	B6 V	16 900	3.72	$38\pm2$	254.45	17 52 14	- 34 47 57	E
6668		162 817	5.96	B9.5 V	9190	3.15	$76\pm4$	258.40	17 54 27	- 34 27 59	E
6878		169 009	6.33	B9.5 V	10 440	3.95	$47\pm5$	105.15	18 23 02	- 10 13 07	E
7337	$\beta^{1}$ Sgr	181 454	4.01	B9 V	11 960	3.83	$77\pm2$	116.01	19 22 38	- 44 27 32	E
8781	$\alpha$ Peg	218 045	2.49	B9 V	9810	3.51	$130\pm2$	42.80	23 04 46	+ 15 12 19	S

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