No.
Remarks
217
Much H emission incl. half
arc outside galaxy. (1)
218
219
Faint arc and filament on N side.
220
221
Faint diffuse material to south, bright filament to hard image on
NW side of nucleus.
222
Amorphous arms. (25)
223
224
Straight filament leads to bright, offset nucleus. (19)
225
Very faint diffuse outer arms, absorption one side of nucleus. (25)
226
Loops, filaments at various angles.
227
Pos. of spiral.SO is E and a little N.Very faint rings extend to
diameter of 7'.4.
228
Defects on blue Survey print in both VV 53 and VV 54.
229
Circular or near circular rings of small density difference.
230
Inner and outer shells visible in direction of axis only.
231
Faintest arc extends about 2' S of nucleus with absorption.
232
Absorption lane reaching away from galaxy.
233
Narrow faint absorption lane in SE direction. (27)
234
Considerable resolution into stars and absorption tubes.
235
Faint outer oval and resolution into stars.
236
Faint outer arm curves around through 270°
237
Knot in arm as large, not quite as bright as nucleus.
238
VV position somewhat uncertain. Double nuclei, N nucleus has third arm.
239
Smaller galaxy is fairly symmetrical spiral.
240
241
242
Very thin, bright tail from north nucleus which has strong
absorption. (15)(17)(19)
243
Some very small bright knots resolved in interior.
244
245
Very faint diffuse connection from both ends of N spiral to S spiral.
246
May not be physically connected.
247
Spirals have common arm, N spiral arm continues NE.
248
Three spirals connected together. (18)(44)(45)
249
Straight connection from faint material on E to middle galaxy.
250
251
Outside arms diffuse and bifurcate.
252
Radio source M09-19.
253
Some resolution of stars or H II regions.
254
Position of brighter galaxy, companion south.
255
Faint arm extends beyond high S.B. companion.
256
Resolution into knots. Note small ragged galaxy W of pair. Radio
source M00-10 is 7'. S.
257
Galaxies joined by segment of thin arc.
258
Resolution into knots on larger galaxy. (15)
259
Material extends SE toward peculiar round spiral.
260
Possibly lines of faint condensations extending south.
261
Some condensations resolved, similar smaller galaxy appears north.
262
Some resolution into knots.
263
Diffuse outer filaments, bright knots inside.
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