Observations of Nebule and Clusters of Stars. 159 
4627 
M. 73 
2093 
2099— 
I. 192 
2098— 
I. Ul 
1851, Aug. 5. Resembles the neb h 2088 though on a much larger scale, the 
dark spaces have a rounder or more sack-like appearance, especially at the 
chief bend, where the neb is also brightest. It has several outlying portions 
of flocculent neby, especially at s end. 
1855, Sept. 3. General shape that of h’s figure [P. T. 1833 Pl. XI. fig. 34], but 
several dark bays in it and many more stars seen in and about it. (IIT. obs.) 
1871, Aug. 24. A few scattered stars. (I. obs.) 
1850. Oct. 1. Net work neb found with ditliculty, appeared quite milky and 
pale with pB centre. 
1851, Aug. 1. EF dash of neby forming background to a few st of milky way; 
Ens, no trace of h’s network. 
1866, Sept. 14. 2 L patches, rather Ens and streaky with many L and § stars 
between them and in their neighbourhood. (IV. obs.) 
1851, Aug. 22. A part of milky way, sev B st about, but I did not see h’s 
neby. (I. obs.) 
1857, Aug. 27. eF, vibM, no Nucl, EH nearly ns. (I. obs.) 
1868, Sept 13. Like a dist glob. Cl, similar to that in Hercules, A 
light mottled, projection p. 
1876, Aug. 15. (3 ft.) B. L. irr R. vvgbM to a very soft by & 
Nucl. Looks H, the Nucl and environs are probably R and 
surrounded by F neby, Espnf, especially sp (extending | 4625 
very little nf). The Nucl seems granular, but sky bad, with lower power it 
looks more diffused, it extends probably over several minutes. 
1876, Aug. 24. Nothing beyond what was seen the other night with the 3 ft. 
Sky hazy. (IIT. obs.) 
1855, Aug. 19. Seen as in sketch. 3 st in it, If neby reaches nearly up to the 
* sf; B knots in it, the nf one seems triangular in shape and sometimes I 
thought it split up by a dark line running from sf to np. [See P. T. 1861 
Pl. XXX. fig. 37.| 
1855, Sept. 3. Seen as before and sketch compared. 
1856, Sept. 6. Details as in sketch confirmed; vB. (VI. obs.) 
1848, Oct. 23. Sketch made. [P.T. 1850 Pl. XXXVIIL. fig. 14.] 
1848, Oct. 25. Sketch confirmed. 
1849, Sept. 16. “Saturn neb.” Pos of ring 81°. 
1850, Aug. 10. The projections faintly seen, the line of anse runs above the 
centre of the neb which fades away pretty gradually. 
1851, Sept. 21. Ansae seen, I suspect F neby all round the neb of about the 
brightness of the ends of the anse. 
1852, Sept. 9. Night far from good, yet with single lens [power about 1300] 
the left ray was separated from the disc being either a patch of neb or a *, 
probably the latter; the right-hand one much fainter, was once or 4wice 
susp. to be a * also. 
1852, Sept. 15. Still impressed with the idea that the p appendage is only a * 
in the outlying F part of the neb. Could not make much of the f app, 
sometimes it was suspected to be separate, at other times I fancied it was 
connected with the dise by a connection sloping on n side in np direction. 
A vS * rather less than a diameter from edge nf. 
1862, Oct. 23. (3 ft.) Saw several times the F st forming the ansae, but I 
think there is F neby about them. 
