DESCRIPTION-(Concluded)

Described as "vL neby, surround star 7 mag."
exposure of 2h 10m. 0 s.n.

Non-existent. No trace in an

Bright elongated patch of nebulosity 0:3 long. It is trinuclear; perhaps a very irregular spiral. It is 1' beyond the longest whorl of 7753, and strongly suggest a satellite nebula, as in the case of M. 51.

A rather faint, symmetrical, open spiral 2:5 long; slightly oval. Nucleus almost stellar and three almost stellar condensations in the whorls. Perhaps connected with 7752. 6 s.n.

Slightly oval; 0.5 in diameter; bright center; slight trace of spiral character.
Slightly oval; l' in diameter. Small, hazy nucleus. The whorls form a nearly
complete oval ring, and are quite faint.

Rather faint p-type spiral 0.8 x 0.4 in p.a. 0°; nucleus almost stellar.
Bright spindle 0:8 long in p.a. 20°; very bright round center.

Rather faint spiral 2' x 1' in p.a. 175°. Nucleus rather bright; whorls com-
pact. 25 s.n.

A sparse, very open cluster of stars of magn. 12-17, 16' in diameter. O s.n.
No trace in an exposure of 2h. Probably can be recorded only in very long
exposures. Described as 30' x 10'. 8 s.n.

Vol. VIII, Plate 70. 3' x 0.8 in p.a. 132°. Bright; no nucleus or whorls are dis-
cernible, but it is doubtless a spiral seen edgewise. A remarkable, clear-
cut dark lane runs down its entire length. See Abs. Eff.
19 s.n.
Moderately bright spiral 3' x 0.5 in p.a. 44°. Small, hazy nucleus; a number
of condensations in the rather compact whorls. See Abs. Eff. 9 s.n.

d

b