Burnham: Measures of Proper Motion Stars 
10061. A. G. 251. (8.6...10.0) 
R. A. 20” n m 51* Decl. + 5 0 49' 
1908.575 
iS 5?4 
7 "20 
• 597 
185.0 
7 -25 
•633 
186.0 
7-30 
1908.60 
185.5 
7-25 
No evidence of motion, 
is much too large. 
The distance 
given in G. C. Part I 
10064. 
Ho 588. (6.5. 
•• 8 . 3 ) 
R. A.20” 
‘ I2 m 7 s Decl.+ 31 0 8' 
A and B 
1907.523 
297.32 
5 o "96 
• 597 
297.13 
50.84 
.638 
297.28 
50.94 
1907.59 
297.24 
50.91 
B and C (12.0) 
1907.523 
17-9 
8'.'79 
•597 
17.5 
8.60 
.638 
15.2 
8.74 
1907.59 
16.9 
8.71 
Early measures discordant. 
10077. 
P 661. (5.7... 
.12.4) 
R. A. 20 1 ’ 12 
: ,n 39 s Decl. + 40° 0' 
1912.583 
.638 
A and B 
64°9 
65-3 
I2"8 5 
12.68 
1912.61 
65.1 
12.76 
There may be a little diminution in the angle since 1878. 
As the proper motion of the bright star is doubtful, I have con- 
nected a faint star. 
A 
and C (13 
• 3 ) 
1912.583 
218!07 
IIl"42 
.638 
217.10 
112.04 
1912.61 
217.58 
in.73 
Auwers 
o?o68 
in 
98 ?S 
Boss 
0.012 
in 
169.2 
Kustner 
0.022 
in 
II 3-5 
10085. x Cephei. 2 2675. 
(4.0...8.0) 
R.A. 20 h 
I2 m 56 s Decl. + 77 0 21' 
A and C (10.1) 
1912.255 
336?6o 
169". 32 
.274 
336.63 
169.48 
.296 
336.55 
169.41 
1912.27 
336.59 
169.40 
The small star appears to be DM (77 0 ) 763 (9.5). 
From the Astrographic 
300''0, we have: 
Catalogue, 
using scale value 
1895 336?3 
170"! 
Greenwich 
The proper motion of x Cephei is given: 
Auwers 
o"oi8 in 
2 4°3 
Newcomb 
0.027 in 
17.7 
Boss 
0.029 in 
25-5 
10100 . 2 2666. (6.5.. 
• 8 . 7 ) 
R. A.2o h I3 m 
52 s Decl.+ 40°2i' 
A 
and C (9.2) 
1908.537 
20 7?6 
34"22 
• 55 6 
208.0 
34.30 
•559 
206.8 
34-44 
1908.55 
207.5 
34-32 
The distance by Tarrant 
is too small. 
1894-59 207 ?4 
34-27 
2n 
Gla 
The proper motion, if any, of the large star is 
small: 
Boss 
o"oi2 in 162 
°7 
10104. v 
Capricorni. 
(4.9... 11 - 7 ) 
R. A. 20 h 
I4 m 0 s Decl. — 13 0 8' 
1908.537 
209?78 
53"90 
• 573 
210.25 
54-24 
• 575 
209.80 
54-22 
•594 
210.18 
53 . 6 i 
1908.57 
210.00 
53-99 
1911.471 
209?63 
54 " 15 
.509 
210.07 
54-21 
• 529 
209.63 
53.89 
1911.50 209.78 54-08 
The four positions by (3 on 10 n (1877-1911) give for the 
proper motion of v Capricorni: 
o"o42 in 2i6?8 
Further measures should be made, as the first of these is on 
a single night. 
The meridian positions leave the amount and direction of 
the movement uncertain: 
Auwers 
o"o24 
in 
2 57°9 
Boss 
0.018 
in 
156.7 
Newcomb 
0.014 
in 
266.8 
10133. Arg. 38. (9.8.. .10.0) 
R. A. 20 h I5 m 25 s Decl. — 20° 37' 
1906.755 272?8 I7?30 
7-675 273.7 17-45 
7.695 273.8 17.43 
1907.37 273.4 17-3 9 
Probably without change. 
255 
