92 



Herman Schultz, 



hl.312 E np to sf ; * ll'"12 in sf part. 



1x1322 estimated much Fr and more diffic April 1871 than in nr equal circumstances 

 Apr. 1865? F * p in the par and F f. 



hl329 E 2' or more np to sf, and ab '/,' br; brightest part by measure in decl-circle 

 = 60"; N irreg and indistinct with evident traces of r ; * 12 ,n s nr on the decl- 

 circle of the N. 



1x1343 E nr in direction of decl. 



It 134.9 E sp to nf in estimated pos = 60°; a trifle Fr than li!343. 

 hl348. GNr? Neby generally Rd and Sr than 1', but momentarily I think it much 

 extended particularly sf? 



hl345 E sp to nf: *a 11'" nf = star of comparison n:o 294. 



1x1350; hl358; It 1359. 



1x1356 Fr than 1x1368; not Sr than '/ 2 ' ; consisting of a v much condens C part, 

 surrounded by Fr neby, both 1 E sp to nf; momentarily radiations even in other 

 directions; obviously though only momentarily r M; *a ll m 12 np, *b 12 m sf. Neb 

 v well seen 1869 April 12. 



It 1358 al Sr and Fr than the f It 1359, with which it forms a dneb, the neby of the 

 two neb momentarily running together ; lt.1358 E sp to nf in pos = 70° a 80° ; v 

 fine «... visible in the neby, but, as the nehy is milky with a blueish fosforescent 

 light, its general appearance indicates no r. 



1x1359 al Br, Gr and more distinct than the p neb; E sp to nf in estimated pos = 30°. 



Rem. These neb obs under v favourable circumstances. S d* 12™13 (dist of 

 components only few seconds of arc) p in the par; an other d* (dist of compo- 

 nents = l) f the neb: np component *a ll'"12, sf 12 ,n . 



1x1357 E 12' a 14', np to sf; pos by measure: 



1870 Apr. 19 ... . 134°,5 (1) 



1871 March 25 . . 137 ,3 (3) 



Neby 7 2 ' br at N, from which it is rapidly narrowing towards the ends; N also E 

 in the axis of the neby, indistinct and not without indications of r; N surrounded 

 by a pretty condens neby, beyond which the light rapidly decreases ; *a 12 m 13 

 nf the N. 



Rem. I have seen that neb under v favourable circumstances: neb consists 

 of two in form and size quite equal parallel branches, separated by a narrow 

 dark canal ; sp branch vB, the nf eF. The n branch certainly eF and only mo- 

 mentarily visible, but then always radiating to the same length as the s branch. 

 N situated at the n edge of the sp branch and consequently just at the border 

 of the dark canal. This canal not quite free from neby. The appearance nr 

 agreeing with the diagr of R. 



