Table 3: Data from the USNO-B1.0 database for objects with non-zero proper motions. N is the number of detections on the scanned plates, and Probab. is the total motion probability.

Object $\mu_{\alpha}$ cos $\delta$ $\mu_{\delta}$ N Probab.

# (mas yr^-1) (mas yr^-1)

36 $+8\pm3$ $+2\pm6$ 5 0.8

44 $-2\pm0$ $-2\pm0$ 3 0.8

45 $+6\pm2$ $+0\pm6$ 4 0.9

47 $-2\pm3$ $+10\pm1$ 4 0.9

53 $-12\pm0$ $+6\pm8$ 4 0.9

55 $-8\pm15$ $+16\pm2$ 4 0.9

57 $-4\pm5$ $+10\pm2$ 5 0.8

58 $+50\pm13$ $-28\pm10$ 4 0.9

**Table 3:** Data from the USNO-B1.0 database for objects with non-zero proper motions. N is the number of detections on the scanned plates, and Probab. is the total motion probability.
Object	$\mu_{\alpha}$ cos $\delta$	$\mu_{\delta}$	N	Probab.
#	(mas yr^-1)	(mas yr^-1)
36	$+8\pm3$	$+2\pm6$	5	0.8
44	$-2\pm0$	$-2\pm0$	3	0.8
45	$+6\pm2$	$+0\pm6$	4	0.9
47	$-2\pm3$	$+10\pm1$	4	0.9
53	$-12\pm0$	$+6\pm8$	4	0.9
55	$-8\pm15$	$+16\pm2$	4	0.9
57	$-4\pm5$	$+10\pm2$	5	0.8
58	$+50\pm13$	$-28\pm10$	4	0.9

Source LaTeX | All tables | In the text

	1 Introduction
	2 Selection of candidates
	3 Observations
	4 General properties of the observed stars
	5 Spectra
	6 Radial velocities
	7 Proper motions
	8 Distances
	9 Analysis and discussion
	10 Concluding remarks
	References
	Online Material
	Appendix A: Spectra