| 
2004— 
VIII. 16 
2058— 
WIUHL, 1G) 
9059 
2060 — 
M. 27 
Observations of Nebule and Clusters of Stars. 
1871, Sept. 4. Cl, st 12—14m, one * 12m rather reddish. (I. obs.) 
1876, Aug. 13. AS group of F st with 2 of 10-llm. (I. obs.) 
1876, Aug. 13. A group of 5 or 6 st 10:1lm anda good many fainter ones ; 
not Ri. (I. obs.) 
1843, Sept. 21. (3 ft.) Very well shown, do not think I can materially improve 
sketch made last year [P.T. 1844 Pl. XIX.] except that I now see more 
stars. Cannot say positively whether resolvable, but see through it an 
immense number of st apparently united with neb* matter. If they are st 
seen through the neb and unconnected with it, it is strange they should be 
so much more numerous than in the adjoining part of the heavens. Exactly 
like the milky way seen with the naked eye. 
1849, Sept. 9. Drawing made. 
| 1849, Sept. 16. Drawing proceeded with, examined also with the 3 ft. to find if 
any evidence of change since drawing in P.T. 1844 was taken ; none decisive. 
[See P.T. 1850, Pl. XX XVIII. fig. 17.] 
1850, Sept. 5. BC Pes, 71" Dist. 180” [Struve’s letters 
Ba 83 150 da 
1850, Sept. 6. By 14 88 de 
| cme 9 128 df 
| pe 6 175 dg 
em) 46 123 dh 
1850, Sept. 7. fr 164 134 dk 
Ep 125 212 dw 
1850, Sept. 9. By jl 83 de 
bo 40 224 db! 
B p 323 222 db 
po 320 175 do 
| Bw 294 116 dp 
Br 244 179 dal 
1851, Aug. 21. Ba 83 165 da 
| pa 294 116 dp 
| Bo 321 184 do 
| B 325 243 db 
| Be 5 195 dg 
1851, Aug. 22. 66 7 141 df 
py 13 88 de 
pb 0 45 137 dh 
Bn 54 107 di 
Bc 60 84 ne 
Bo 4] 243 db! 
BA 246 114 Ba 
BE 74. 187 de 
A is the extremity of the B mass of neby in the sp quarter. 
1851, Aug. 24. 6X Pos. 86° Dist. 162” ([Struve ... 
Br DAG 185 da’ 
| Bw 207 180 
Bo 212 172 
B A 250 107 000 
| po 321 176 do 
| Bw 346 49 a 
pK 164 147 dk 
| Bp 125 223 dw 
Biv 110 286 dr 
|| For Struve’s observations see P. T. 1861, p. 739-40. The above Position 
angles have been corrected by supposing an interval of about 24™ to have 
elapsed between two consecutive measures. See P. T. 1861, Pl. XXXT.] 
