Burnham: Measures of Proper Motion Stars 
113 . Hd io. (10.7.. .11.3) 
R. A. o h n m ± Decl. + 3°4 , ± 
1908.652 237?4 31"52 
•655 239.0 30.97 
.709 238.8 31.21 
1908.67 238.4 31.23 
The note in the General Catalogue as to this pair following a 
7.5 m star, belongs to Hd 13 (No. 124) as given in Part I. The 
distance of Hd 10 in the measure of 1903 is much too large. 
116 . 38 Piscium. 2 22. (7.0...8.0) 
R. A. o h n m 13 s Decl. + 8° 12' 
A 
and C (12.5) 
1910.684 
I 4 i ?82 
63-51 
.701 
142.20 
63.75 
• 703 
141.88 
63.86 
1910.70 
141.97 
63.71 
136 . PI 1951. (8.0... 12.0) 
R. A. o h i2 m 4i s Decl. — ii°37' 
1908.633 2i8?4 22"87 
.652 217.7 22.98 
.655 216.5 22.95 
1908.65 217.5 22.93 
The only earlier measures are my own, given in G. C. Part II. 
As the first position depends upon a single night, the apparent 
change in distance may not be real. 
141 . t Ceti. H 1953. (3.7...12) 
R. A. o h I3 m 19 s Decl. — 9 0 30' 
1910.666 
i6?90 
63"74 
.681 
17.08 
63.02 
.701 
16.95 
63-58 
1910.68 
16.98 
63.45 
For proper motion of AB. Other values from meridian 
positions are: 
Auwers 
0"109 in 
20?0 
Boss 
0.120 in 
44-9 
Hedrick 
0.074 in 
102. I 
118 . 
223. (7.6... 
9 - 9 ) 
R.A. o h 11 
m 20 s Decl. 
— o°2i' 
A and B 
I 9 II- 54 S 
329? 1 
4 " 7 i 
• 564 
328.6 
4-58 
• 583 
329-3 
4.86 
1911.56 
3290 
4.72 
This, with the prior measures (1836-1911), gives 
for the 
proper motion of the principal star: 
o"i2i in I5°i 
The movement from meridian positions 
is: 
A. G. Nico. o"ii2 in 
0° 
For a further independent value, I have connected 
a faint 
star: 
A and C (11.6) 
1911.545 28i?40 
I 03 "i 8 
.564 281.30 
102.95 
.583 281.30 
103.25 
1911.56 281.33 
103.13 
119 . Hd 11. (9.8.. .10.7) 
R. A. o h 1 i m 39 s Decl. + 3° 5' 
1908.633 290?5 
36 " 4 i 
.636 291.4 
36.34 
.652 291.0 
36.60 
1908.64 291.0 
36.45 
It was obvious that one or the other 
of the prior single 
measures given in G. C. Part II of this 
star must be 
wrong. 
The distance in the measure of 1903 is about 1" too large. 
Comparing this with the first position in 1880, we have for 
the proper motion of 1 Ceti: 
o'.'o72 in 243?8 
Other values from meridian positions are: 
Auwers o"o49 in 237^9 
Boss 0.037 in 209.0 
Newcomb 0.035 in 212.5 
144 . S 3S4. (6.8...9.3) 
R. A. o" I3 m 44 5 Decl. + 37 0 34' 
1910.666 
I 9?30 
71-39 
.678 
18.83 
71.29 
.681 
18.90 
7 i. 3 i 
1910.67 
19.01 
71-33 
The proper motion of A from the measures of AB, and from 
the star catalogues is : 
Measures 
o"309 in 
206? 1 
Stumpe 
0.332 in 
207.0 
Porter 
0.304 in 
211.9 
There is no indication or probability that the smaller star has 
any sensible proper motion, but I have measured a much fainter 
and nearer star: 
A and a (13- 5 ) 
1910.678 
267°. 0 
20" 78 
.684 
266.5 
20.30 
■ 739 
267.5 
20.73 
1910.70 
267.0 
20.60 
158 . Hd 
14. (9.5.. 
• 13 - 5 ) 
R. A. o h i5 m 
12* Decl. + 7 0 22' 
1907.772 
I 57°3 
5 i"i 3 
9-703 
158.6 
51-50 
1908.74 
158.0 
5 i. 3 i 
No other measures of these stars. 
79 
