80 



Herman Schcltz, 



11.616 pretty B; has many *... nr: * ll ,n 12 sp, *a ll m 12 nf, * 9 m ,4 sp 21 s , *9 m ,5 

 f 10" and 3' n. Seems not to have been reobserved since H s time. 



1x4:81: * 10 m ll sp; neb has a conspicuous N 12 m , which seems momentarily to r. Neb 

 generally has the character of r, but not sufficiently well seen for deciding. R 

 has: "Centre r?" Comp also SN! A vvF neb nf It 481? 



h482 evident ®, rr; * 1 2 "13 sp (nebs?), which has 2 other *... 10 n ll and ll m sp. 

 Rem. SN has: "Cumulus admodum coarctatus"; R says nothing of the r. 



h495. Neby insignificant, E nr in the decl-circle np to sf; v indistinctly seen. N 

 momentarily r. 



h497 indubitably "B , distinctly though not constantly rr; obtuseang J with 2 *... 

 11'" n and sf. R says nothing of the r. 



GC.1644, 1650 = B'A Novcb noticed and observable, though not yet obs. 

 h500 al Rr than 1,501. 



11.259 considerably Br than It 507 : * 9 ,n 10 nf; many more in the neighbourhood. 



Rem. GC has "r", but the neb seems now to be entirely without the cha- 

 racter of r. Neb not obs by D'A and, as far as I know, first in Upsala reob- 

 served since H s time. The new position not very well according with H s . 



1x507 in a region rich in «... ; poor *gr sf . As C, though F, is stell, the measures 

 should be better accordant; perhaps more *... than one in C? 



h526; GC. 1705; h527. 

 h526: * 12"13 nf, * 13™ sf, neb J with 2 *... 10 m . 



GC.1705 vvS, nf att to 1/526; once the two seen distinctly separated, but no posi- 

 tion taken. GC quite right; R erroneously identifies GC.1705 with It 527. 



h527 eF but 1865 March 19 indubitably seen nr in the place of GC, yet too diffic 

 for obs; probably ®. Neb of the same faintness immidiately nf? 2 10 ra lln 

 and sf. No more neby here seen. Comp SN! 



Ii530 looks like * 10 ra ll with F nebs atmosphere hardly Gr than '/„' ; d* ll m p, 

 * 12 m f, which *12 in fs. Sky v light. 



Rem. h says "* with vF extensive neby"; R: "nucleus surrounded by v ex- 

 tensive neby"; D'A and Rumher respectively make the diam 60" and 150". 



7^55^ E 4' in 42° pos, '/<>' br at N; planetary N 2" situated in the Br n part of the 

 neb, forms nr isosc J with 2 f «... . The neby nr extends to the n of these stars 

 (ll m 12), which however is not exactly on the central-line of the neby. The dist 

 bet this * and N perhaps nr half the length of the s part of the neby. 



