Burnham: Measures of Proper Motion Stars 
1859. 29 Tauri. II 2004. (5.5... 12) 
R. A. 3" 39“ 17* Decl.+ 5°4i' 
1906.772 
64?! 
64"72 
.796 
64.0 
65 -39 
.813 
63.8 
65-74 
1906.79 
64.0 
65.28 
No early measures. The proper motion of the large star is 
uncertain: 
Auvvers o"oi4 in 23g!6 
Boss 0.030 in 115.8 
1860. H 1139. (7.4...9.1) 
R. A. 3 h 39 m 20 s Decl. + 70° 7' 
1909.742 
175 ° 1 
47"24 
.760 
175 .1 
47.20 
•763 
175-2 
47.09 
1909.75 
175 -i 
47.18 
B is the 9.3 m star, DM (70°) 263. 
The only other measure is of late date. The proper motion 
of A is given: 
Schroeter 0^056 in 2o8?9 
A and C (13.5) 
1910.701 
37-5 
ii 1 
’.'60 
.703 
39-5 
11 
.69 
• 739 
39-4 
11 
.82 
1910.71 
38.8 
11 
.70 
A is the brightest star in h 308; the others much smaller. 
No change in AB. 
The principal star is given a small proper motion: 
Battermann o"o48 in 221 ?7 
1882. P 1184 
R. A. 3 h 41 m 14 s Decl.+ 22 0 0' 
About 10' distant from this pair sp, is a nebula discovered by 
Lohse (Dreyer 1456) about a pair of faint stars I30°:9"; 
“ companion nebulous.” In measuring this pair, I could not see 
any trace of a nebula in the field. The magnitudes of the stars 
were estimated 10.8 and 11.5. 
1909.760 i30?9 9"36 
.938 130.2 9.54 
1909.85 130.5 9.45 
1886. 30 Tauri. 2452. (4.5...9.6) 
R. A. 3 h 41 m 41 s Decl. + io° 46' 
1861. H 665. (9.8...10.0) 
R- A. 3 h 39 m 23 s Decl. + 30° 26' 
A and C (11.3) 
1909.706 
2 S 5°6 
I 4"79 
.782 
255-9 
15.ii 
.838 
256.0 
15.22 
1909.78 
255-8 
15-04 
I 9 H -947 
59°4 
9"io 
11.950 
59-0 
9.18 
12.008 
57-8 
9.12 
1911.97 
58.7 
9 -i 3 
The proper motion of 30 Tauri is very uncertain in amount 
and direction. From meridian positions: 
Auwers o"o22 in 199^3 
Boss 0.042 in 121.9 
The only other measure is given in G. C. Part I. 
1869. 2447. (7-8. ..9.5) 
The measures of the faint star show that the motion of A is 
nearly all in R. A. From the observations of 2 , A and P on 
12 n (1830-1911) we have: 
o"oo4 in 283?5 
R. A. 3 h 40 m 8 s Decl. + 37 ° 58' 
1911.663 
i 67?35 
28 "23 
.720 
167.42 
28.13 
.736 
167.38 
28.13 
1911-71 
167.38 
28.16 
The principal star has a small proper motion. From 
measures of 2 and P (1836-1911) this is: 
o"o 62 in 2SF0 
1888. 2 456 rej. (8.5... 9-3) 
R. A. 3" 42™ 10 s Decl.+ 1° 13' 
1909.936 II9?0 22"o5 
10.701 II9-9 21.69 
the 10.739 120.3 21.60 
1910.46 II9-7 21.78 
No change apparent from the measures. 
1877. 2446. (7.0...9.2) 
1896. A. G.74. (9-3-•-9 5 ) 
R. A. 3 h 40 m 25 s Decl. + 52 0 17' 
R. A. 3" 42 m 49 s Decl. + 12 0 33' 
A and B 
1907.772 
195-4 
11 
-'45 
1910.701 
254-0 
8"73 
co 
195-9 
11 
.91 
.703 
253-8 
8.78 
.791 
195-6 
11 
.96 
• 739 
253-9 
8-37 
1907.78 
195.6 
11 
•77 
1910.71 
253-9 
8.63 
Prior distances discordant. 
118 
