( 264 ) 
Besides, the stars with a total yearly proper motion > 0".3 have 
been left out too. 
Combining the values of A ges for both parts of each belt, according 
to their weights, the result is: 
A. sin x > + 0.80 corr. A ws prel. corr. | total corr. Apz 
Southern Declination — 0".0093 (226 st.) | — 0.0080 — 0".0173 
Decl. 0° tot + 20° — 16 (215 ») | — 80 — 96 
» +20° » 40° ~ 34 (258 ») — 80 — 114 
> +40° » + 60° — 2 (160 ») | — 55 — 57 
» -+60° » + 900 — 17 (95 ») | — 10 | En 7 
numb. of stars 954 | 
B. + 0.80 5 sin x > + 0.50 corr. A ps | | total 
South. Decl. — 0".0024 (278 st.) | — 0",0080 — 0.0104 
Deel. 0° tot + 20° — 90 (218 ») — 80 — 170 
» 209 » +400 = 52 (181 ») = 80 = 132 
» +40° » + 60° — 5 ( 62 ») | — 55 — 60 
» + 60° » + 90° + 42 ( 32 ») | — 10 aa 32 
numb, of stars 721 
The combination of the values sub 4 and B, with weights pro- 
portional to sin? z (n=number of stars), is given in the following 
table : 
C. sinx > + 0.60 Aps | prel. corr. ; Total Ags | prob. err. 
Scuth. Decl. — 0.0062 (504) | — 0”,0080 | — 07.042 | 070015 
Decl, 0° tot 4-200 oi "445 (438) — 9 BO ads 93 
pi B00 > got Ae RY Seedy) = KBO EN 16 
pi? ee ee 1 (922) a 55 | ee tee 13 
» 260° pi. 90%. Be vn BT [oy AD | ik 0 20 
numb. of stars 1675 
What part is due to each Spectr. Type in making up these 
final values, is shown in the next table: 
