----------+--------+-----+-------+-------+-------+

+--+---------------------+------+--------+---------+---------+----+------+
| 1| 2 | 9 | 10 | 11 | 12 | 13 | 14 |
+--+---------------------+------+--------+---------+---------+----+------+
| | | Motion | Magnitude | Spectrum |
| | _Name_ +------+--------+---------+---------+----+------+
| | | [mu] | _W_ | _m_ | _M_ |_Sp_| _m'_ |
+--+---------------------+------+--------+---------+---------+----+------+
| | | |sir./st.| | | | _m'_ |
| 1|Barnards star |10".29| -19 | 9m.7 | +11m.7|Mb |11.5 |
| 2|C. Z. 5h.243 | 8.75| +51 | 9.2 | +10.1 |K2 |10.6 |
| 3|Groom. 1830 | 7.06| -20 | 6.5 | +5.0 |G5 | 7.6 |
| 4|Lac. 9352 | 6.90| +2 | 7.5 | +8.2 |K | 8.9 |
| 5|C. G. A. 32416 | 6.11| +5 | 8.2 | +8.5 |G | 9.1 |
| 6|61 Cygni | 5.27| -13 | 5.6 | +6.5 |K5 | 7.2 |
| 7|Lal. 21185 | 4.77| -18 | 7.6 | +9.1 |Mb | 8.9 |
| 8|[epsilon] Indi | 4.70| -8 | 4.7 | +5.4 |K5 | 6.3 |
| 9|Lal. 21258 | 4.47| +14 | 8.5 | +8.5 |Ma |10.3 |
|10|O^2 Eridani | 4.11| -9 | 4.7 | +4.3 |G5 | 5.8 |
|11|Proxima Centauri | 3.85| .. | 11.0 | +13.9 |.. |13.5 |
|12|Oe. A. 14320 | 3.75| +61 | 9.0 | +5.1 |G0 | 9.9 |
|13|[mu] Cassiopeiae | 3.73| -21 | 5.7 | +4.4 |G3 | 6.8 |
|14|[alpha] Centauri | 3.68| -5 | 0.3 | +3.2 |G | 1.2 |
|15|Lac. 8760 | 3.53| +3 | 6.6 | +7.0 |G | 7.5 |
|16|Lac. 1060 | 3.05| +18 | 5.6 | +5.1 |G5 | 6.7 |
|17|Oe. A. 11677 | 3.03| .. | 9.2 | +9.1 |Ma |11.0 |
|18|Van Maanens star | 3.01| .. | 12.3 | +12.7 |F0 |12.9 |
+--+---------------------+------+--------+---------+---------+----+------+
| | | |sir./st.| | | | _m'_ |
| | Mean | 5".00| 17.8 | 7m.3 | +7m.6|G8 | 8.7 |
+--+---------------------+------+--------+---------+---------+----+------+

That the great proper motion does not depend alone on the proximity of
these stars is seen from column 10, giving the radial velocities. For
some of the stars