158 Observations of Nebule and Clusters of Stars. 
| hen | 
4598 2086— | 1857, Aug. 1. D*f closely, exactly in a line with it, the larger * being nearer 
Til. 219 to the neb. Nearly R, vy S,1bM, edges very indistinct. (I. obs.) 
4600 2088— | Nebula near k Cygni; examined about 20 times, but only rough sketches made. 
Wo 1G Deferred for further examination. 
4601 | 2087= ) | 1857, Aug. 27. Group of 5 neb, very many st 
IT. 426 among them. ais1H,bM; bisS, nearly R, 
4602 | bM; ¢ is 1 EK, bM and has a conspicuous * 
4603 |-| R. novee > closely nf; d is about 7’ or 8’ dist. from a, 
4604 | and is pF, R, bM; eis 8S, R, bM, *sf [d= 
4605 | 2089=— h 2087, e=2089]. 
II. 427 J) | 1857, Aug. 28. 5 neb seen, last night’s obs. 
confirmed. 
1873, Sept. 28. 
*10m to neb(1) Pos. 87°-1 Dist. 186"-0 
Same * to neb (2) 51:9 135-6 
(1) is F, R, gbM [4605 =e], has a * 12m in Pos. 
121°-6, Dist. 42-6; (2) is F, R, gbM 
[4601=d]. A pB, Rneb, gbM in Pos. 55°:9, 
Dist. 236-1 from (1) has a * 13m np and 
another * 13m sp, both incontact ; possibly the 
whole is only a triple * ; definition very bad. 
1876, Aug. 14. Found a v F,vS stellar neb, 
sp in Pos. 207°-3, Dist. 288'-9 there is another p F, v8 with 2 F st v mr, it 
may itself also be a F *. Perhaps there isa v F,vS neb bet the 2 objects, 
a little f, forming an isosceles A with them. Clouds came on. 
1876, Aug. 23. Measures from 4601 (p F, p 8). [4] 
4605 F,S Pos. 134°:2 Dist. 112'°5 has a* 14m 3+ sf 
4602 v F,S 322°7 194°8 [observed by @’A., =a] 
4604 vF,vS 35°8 SHY) [=a] 
The last neb has a * 10m in Pos. 87°:5, Dist. 48'°5. A vvF neb a few minutes 
s of last neb is very doubtful. I had no time to look carefully. (V obs.) 
5975 508 1873, Aug. 20. Nebulous *, neby cE pf, a=20" 45™-5, NPD=59° 50'+ (1. obs.) 
4607 II. 206 | 1866, 1871, 1876. 3 times not found. 
1873, Aug. 16. eFneby, fs end are 4 F st forminga S are. * 9°5m Pos, 226°-2, 
Dist. 216"-9. (1. obs.) 
4608 2090— | 1852, Sept. 9. The outlying parts seem extensive and m E npp sff. 
M. 72 | 1873, Sept. 26. Glob. Cl, very much compressed to at least 2 centres. Measures 
taken as nearly as possible from the middle of the whole Cl. 
* 10m Pos. 166°°4 (2) Dist. 134" (2) 
 1@) 175-2 (2) 197 (2) 
8 113°8 (2) 168 (2) 
* 12 47-2 118 
1875, Sept. 8. S glob Cl, st 13:14m not vmeM, irr fig. 
* 12m Pos. 162-1 (2) Dist. 130” (2) 
* 12m 175:2 (2) 192 (2) 
* 10m sff 31’ dist, * 10:-11m f 4' dist, sev fainter ones about. 
1876, Aug. 11. (3 ft.) The * sf isin Pos. 167°1 (3). [Some mistake made 
in 1875.] (V. obs.) 
4616 2092— | 1849, Sept. 12. Formed of wisps of which the general direction is in length of 
Wo id! neb and which in many places make a kind of network ; the brightest part 
of the neb is nearer n end and is 7’ or 8’ broad. I saw none of the decided 
forked forms of h’s drawing, but I did not examine this very closely ; yet near its 
southern end two of the wisps are vl, their junction being sf. This perhaps 
was what h saw. General direction of neb in npsf. 
