Observations of 500 Nebulae. 



75 



1x39 E in the decl-circle. 

 h41 Q. 



1x43 an indistinct but not eF object; not obs. 



h44, 1x50 only once obs; obs of small value, the sky being too light. 



11.857 less F than GC.103 (seen but not observed). 



1x40 inconsiderably Br than h23, but no doubt Br than II. 857 and 11.858. 



11.858 less F than GC.103, nr as 11.857. 



GC 5058: *all'" immediately sp, which makes the obs of that vvF object e diffic. 

 GC.119 in straight line bet 2 * ll ffl np= *a (GC. 5058), * 10»11 sf. 



h 59 has * 10"' nf — neb 1' n from that *? Neb also suspected p in the par of h 59 

 and also immediately nf. 



Rem. The other neb of this vicinity could not be verified with certainty, 

 although the state of the air at least once pretty favourable. They are no doubt 

 eF. Comp SN! 



h65 rr with magn. p 210; no essential C condens, but Br * nr M. 

 1x78 A with 2 *... 10"' sf and 12" 1 nf. 



R.Novce not in my working-list, and not noticed. Comp SN! 



h84;h85; h86 = R. a, /?, y; S and nr O; h86 the brightest. 

 GC.205 = R. y considerably Fr and Sr than the 3 np; *a ll m sp. 

 GC.207 ; GC.208= R. cr, t; S and CJ; pretty good for obs even in moonlight. 

 GC.209; GC.210=R. S, 0; not found. Comp GC and SN! 



GC.199 long and carefully searched for in vain 1867 Oct. 30. Strong aurora, 

 GC.217 not v diffic but for 2 10'" sf. 



h87 and nf GC.215 nr equal — GC.215 at the time not obs. 

 GC.213 identical with GC.215. Comp SN! 



h 89 r M. State of the air always iufavourable. 



Novalllsp 11.220 : da = 0,4 min, zM = l',5; 2 *... p : 12"' n and 11™ s. 



11219 p exactly in par of 11.220 : z/« = 0,l min; stell. The eF neby several times 



verified is indubitable. 

 II.220-.N v indistinct; r? 



NovalV sf 11.220 :Aa =0,3 min, AS=2\3; 2 *... 11'" f. 



Rem. The identification here hypothetically adopted agrees with GC and 

 with II:s remark (11.219; 11.220): "preced faint vS; following pL". But it 

 nevertheless seems astonishing and worth remarking, that H has noticed the eF 

 and often doubtful neby of 11. 219, and yet should not have seen the relatively 

 B Novae. Can this peculiarity be owing to some variations of the objects in this region? 

 JD'A has here only 2 neb, and identifies 11. 219 with the first Nova. 



