Burnham: Measures of Proper Motion Stars 
C and G (n.3) 
1908.444 
U9?8o 
I3 o "78 
.460 
119.80 
130.44 
•479 
120.01 
130.67 
.482 
119.89 
130.97 
.518 
H9-54 
130.63 
1910.260 
120.75 
129-55 
• 299 
121.25 
130.22 
-337 
121.07 
129.79 
• 356 
121.35 
129.82 
• 375 
121.40 
129.64 
1908.460 
C and H (12.1) 
29H0 
i63!'o7 
-479 
29. xo 
163.02 
.482 
29.30 
163.21 
.518 
29-15 
163.00 
1910.260 
28.58 
160.02 
■ 299 
28.92 
159.96 
• 337 
28.50 
160.27 
•375 
28.83 
159-93 
• 395 
28.45 
160.12 
1908.479 
C and c (13.6) 
52°03 
63"23 
.482 
52.07 
63.14 
.518 
52.88 
63.XI 
1910.260 
52.50 
60.10 
• 279 
51-55 
60.07 
•337 
52.03 
60.08 
■ 397 
52.50 
59-44 
1910.444 
E and G 
6o?32 
H3"37 
.460 
60.20 
113-59 
• 479 
60.45 
113.64 
.482 
60.47 
H3-77 
.518 
60.05 
113.91 
1910.260 
60.23 
H3-37 
• 337 
60.30 
114.02 
•375 
60.43 
113.66 
•395 
59-98 
II3-9I 
1908.460 
A and E 
116! 47 
i5o'.'88 
• 479 
116.66 
150.91 
.482 
116.50 
151-19 
.518 
116.20 
150.65 
1910.299 
116.52 
150.52 
•356 
116.65 
150.44 
•375 
116.33 
150.58 
• 395 
116.35 
151.40 
The mean results of the two sets of measures of the small 
stars around C are: 
CE 
1908.48 
173-26 
I22"6o 
4 n 
1910.32 
174-43 
124.31 
5 n 
CG 
1908.47 
119.81 
130.70 
5 n 
1910.32 
121.16 
129.80 
5 n 
CH 
1908.48 
29.16 
163.07 
4 n 
1910.33 
28.81 
160.06 
5 n 
Cc 
1908.49 
52-33 
63.16 
3 n 
1910.32 
52.14 
59-92 
4 n 
EG 
1908.47 
60.30 
113.66 
5 n 
1910.34 
60.24 
H3-74 
4 n 
AE 
1908.48 
116.46 
150.91 
4n 
1910.36 
116.62 
150.74 
4 n 
As would be expected, there is no change in EG, and none in 
AE except that due to the motion of A. From the four stars 
connected with C we have for the proper motion of that star: 
CE 
R. A. + i "255 
Decl. + 1 "070 
CG 
1-340 
1.318 
CH 
1.265 
1.162 
Cc 
1.470 
1.000 
1-333 
1-137 
Therefore the annual proper motion of C is: 
1-752 in 49? 5 
The agreement with the former result from the measures of 
AC is all that could be expected when it is considered that the 
time interval is less than two years. 
9093 . Schj 19. (8.6...9.0) 
R. A. 19" 5" 1 57 s Decl. + o° 43' 
1909.531 257?63 5o"49 
.534 257.80_5Q-37 
1909.53 257.71 50.43 
Hind’s nebula about 15' distant np is large and diffused, with 
no definite point for measurement; might be a cluster of very 
faint stars. 
9094 . 2 2477 rcj. (8.5...10.5) 
R. A. 19” 6 m o s Decl. — 4 0 40' 
1911-548 
45-5 
27'-59 
.564 
45-2 
27.46 
•567 
45-8 
27.80 
1911.56 
45 ■ 5 
27.62 
Further measures are needed to confirm the apparent change 
shown by the single measure of Mitchel in 1848. 
9116 . 
(3 139- (6-7-• 
.8.0) 
R. A. I9 h 
7 m 12 s Decl. + 16 0 39' 
AB and C (7.5) 
i9 IT -334 
285?70 
xi4"66 
• 356 
285.30 
114.56 
-373 
285.53 
H4-73 
I9II-35 
285.51 
114.65 
From five positions on 14 n by A, Fr, A and |3 (1874-19x1) 
the apparent motion of C is: 
0^234 in 150?7 
Therefore if the meridian value is correct, AB has no 
sensible motion. To test this, I have connected faint stars with 
each. 
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