* 



90 Herman Schultz, 



1i1228: diam ab '/„'; * 12™ np ; * 9™ nr on the decl-circle of neb, 2' a 3' n ; * 5/(124) sf. 



hl232 rN 4" a 5"; diam ! / 2 ' a 2 / 3 ' ; bet 2 12 m np and 11™ sf. 



Rem. 111.97 not inserted in my working-list and not seen. 



U1237; It 1250: hl244; GC.2065; hl253; U1267. 



hl237 bet 2 a and 3 d order of B; 6 N with evident traces of r; v ill seen, the sky 

 being much too light. 



hl250. Identification according to Sf and D'A. Neb has perhaps sev *.,. in M? Sky 

 much too light. 



hl244 ab '/,' br in the decl-circle and ab 1' lg in the par; Frthan Itl250; C condens 

 large and indistinct. Neb well seen 1865 Febr. 27; I then noticed no traces of 

 r, which on an other occasion I thought that I perceived. 



GC.2965 not seen; sky too light. 



hl253 much resembles hl237, and is hardly Fr than this neb; N of hl253 is even 



Br and distincter; no C r remarked — sky too light. 

 hl267 hardly Fr than hl244; at least momentarily seen E in pos ab = 30°; *12 m np. 

 Rem. This region, so rich in neb, is not yet sufficiently examined. 



hl239: * 9™,5 sf. 



hl242 am the faintest of the 2 a order; *a 9 m ,7 sf and *b 12™ nf; neby at least 2' 



and 1 E in direction of *b inv; neby also momentarily seems to extend to *a. 

 1il251 1 E np to sf. 



It 1258 only once seen under v unfavourable circumstances. Neby much E np to sf; 

 N indistinct, diam 2" a 3". 



U1268; h 127 2; hl27G. 



hl2G8 once seen; v diffic, as sky tolerably light; Gr than the f neb hl272; * 13 ra 14nf. 

 It 1272 rather more diffic than the p neb, obs on same occasion; * 12™ np troublesome. 

 hl270: diam '/ 2 '; B and easily obs. 



hl274; It 127 5; h!287; hl290. 



It 127 4: diam ab l / 3 '; equal to hll48: of the same B, but a little Sr. 

 It 127 5 Gr than It 127 4. 



h!287 remarkably Fr than h!290; * 10™ nf. 



hl290: diam ab */,' E sp to nf; a little Fr than 11.114 and 115, but remarkably Br 

 than M287 ; N G and not stell. 



hl28G: diam did not appear Gr than sky v light; N stell. 



