KUNGL. SV. VET. AKADEMIENS HANDLINGAR. BAND 43. N:o 10. 21 
List of Objects. Plate 4. 
Right 
3 å Annual Declination Annual SEINE 
Object Ascension, pra 1900.0 PrecösS Description. 
1900.0 
60. 4532” 19 BAN T7S fräåsinol KF 220060 + 9.6 »Dumbbell Nebula», Messier 27, according to 
Herschel »very bright, very large, binuclear, irregularly 
extended.» 
The appearence of the nebula is the generally 
known, with the polar nebulosities well marked. 
NEGSC: 702621 32155 CFI2067 = 47126:7 "+ 14.3 Discovered by Burnham 1873 (Monthly Notices 
52 p. 45), »pretty bright, binuclear, planetary.» 
The original plate shows the nebula to be binuclar 
and probably of the Dumbbell Nebula type with large 
polar nebulosities). No other nebula of this type is 
; known. 
N.G.C. 7026 » » » » Reproduction of the same object on a smaller scale. 
EICT298 NEN Sar FR Pa! NS. »Faint, large, little extended, very gradually little 
brighter in the middle.» 
The appearance of the nebula is almost that of a 
l spiral-nebula. 
G0 801 JGA 60390 FOR » Planetary, pretty bright, pretty small, very little 
| extended, 1' diam.» - 
A very regular ring-nebula. 
EGX0P1225 ao FRISSAN OMuDOrLS 121 » Planetary, pretty bright, very small, very little 
extended.» 
Small, little extended nebula, almost uniform with 
defined border. The original plate Shows it to be a 
dense regular ring nebula with a minute nucleus, seen 
projected on the side. 
GEO! 1532 HäP238D FFS SIG REEF BIN — f30 » Bright, small, round; star 9 m in the middle.» 
Very bright central body, with a lateral jet of 
nebulousity. 
G. C. 1546 TrSOM2IVEE 395 SDR 2OI— 7.6 » Pretty bright, considerably small, very gradually 
very little brighter in the middle, resolvable, almost 
planetary.» 
From three plates this object appears to be a 
partly visible ring-nebula. The visible part is little 
deformed, and surrounded by fainter and irregular 
nebulosities. A pretty large nucleus is perceivable. 
GNOTR8T 032 338 FF 31 + 54 1.3 — 18.6 » Considerably bright, pretty large, round, very 
gradually, very suddenly much brighter in the middle, 
nucleus 135.» 
Bright centre, from which a curved wisp issues. 
Faint stripes of nebulosity surround the brighter part 
of the nebula. The centre proves to be trifide. 
