Observations of 500 Nebulae. 



91 



hl288; 11.630; U1295. 



hl288: diam ab 2 / 3 '; sev *... visible in N; a little Fr tban 11.114 and 115. 

 11.630: diam '/,'; E sp to nf ; considerably F and diffic; neby milky with a dull N 4" a 5". 

 hl295 not much Fr than U1288; diam hardly '/„'; neby and the G N both E in the 

 par; C r suspected but not seen. GO really has "r". 



h 1292; StruveNova; U1293; 1x1294; hl305. 



M292: diam •/,' ; am the brightest of the 4 th order, and Br than hl305, which be- 

 longs to the normal neb of that order; 2 *... ll m 12 f n and s. 



StruveNova sp It 1294 : da= 16 s , Jd = 2S"; not eF, but * 12™ just sp, makes it v diffic. 



hl293 E nr in the decl-circle; N G and dull, has a nr planetary appearance; Fr 

 than h l292 and hl305. F neb 2' n 3 s f? 



hl294 evidently @; diam 3' a 4' at least, but extreme parts of the neby vF; brightest 

 C part by measure = 80"; N irreg and resolved in sev B stell points, which toge- 

 ther make the impression of * 10 " or 9 "10; the remaining C part also momenta- 

 rily resolved into e fine *... mingled with neby; *a ll in f exactly in the par. 



hl305 pretty B, but *... 10 m ll sf and nf v troublesome. 



Rem. Neby suspected at sev points of this not yet sufficiently explored 

 region. 1871 in April : it was remarked, that both the neb h 1292 and k 1293 were 

 miiky and of a blueish colour without character of r ; 1865 in April :h 2193 was 

 on the contrary suspected to be © • 



11.114; 11.115; 11.116. 



11.114. Neby vF and al Gr than 1'; N 2", distinctly but not steadily r with magu 

 p 320; makes an isosc A with 2 *... s, 1 1 1,1 1 2 p and 11™ (double) f. 



11.115 much of the same character as 11.114; perhaps not quite so B but al Gr ; 

 N 3" distinctly but not steadily r with magn p 320. As N of 11.114 was re- 

 solved into sparkling stell points, N of 11.115 divided into nebs or dull pla- 

 netary knots. 



II. 116 am the brightest of the 5 th order ; diam '/„' a 2 / 3 j E sp to nf ; the large N 

 has no traces of r. 



Rem. Respecting the r of these objects comp SN! 



h!296; hl298; hl301. 

 hl296: diam ab '/,'; al Fr than 11276. 



M298 remarkably Br than M296; by measure diam = 41" ; evidently : sev stell 

 points sparkling through the neby particularly in its n part. 



hl301 the brightest of these 3 neb; ® with many stell points sparkling through the 

 neby around N, looks v indistinct; by measure diam = 103." 



1x1307 remarkably Fr than hl242; diam ab */,' ; evident traces of C r. 



