Arp 24
Arp 34
Arp 34: the northern galaxy
Arp 34: the southern galaxy
Arp 72. The long tail to the east is not really
visible in this image, except for some blue clumps far from the main disk.
Arp 82
For more images of Arp 82 at other wavelengths,
click
here.
Arp 84
Arp 85 (M51)
Arp 87
To see an Hubble Telescope image of
Arp 87, click
here.
Arp 89
Arp 91. North is up and east to the left.
There appears to be a short blue-ish tail to the
northwest of the western galaxy. This may be caused by
star formation in gas that
flowed from the eastern galaxy (the bluer spiral), to the
western elliptical-like galaxy (w/ a yellower color), and overshot
its target (as in the northern tail of
Arp 285. Alternatively, it may be a tidal tail of the spiral
galaxy that happens to be behind the elliptical.
Arp 101
Arp 103
Arp 104
Arp 105
Arp 107
For more images of Arp 107 at other wavelengths,
click
here.
Arp 112
Arp 120
Arp 136
Arp 173
Arp 181
Arp 194. Notice the bright blue stars in the bridge.
Arp 192
Arp 202
Arp 205
Arp 205: eastern galaxy, close-up
Arp 240
Arp 242
Arp 269. North is up and east to the left.
Notice the bright blue stars off-center in the northern galaxy.
These may have formed from gas accreted from the companion.
Arp 270
Arp 280
Arp 280: Closer view
Arp 283
Arp 285
For more images of Arp 285 at other
wavelengths, click
here.
Arp 285: Northern galaxy (NGC 2856)
Arp 285: Southern galaxy (NGC 2854)
Arp 290
Arp 290: Northern galaxy closer
view.
Arp 290: Southern galaxy closer view.
Arp 294
Arp 294: Closer view
Arp 297. Note that this is two separate unrelated
pairs at different redshifts, with the pair to the north
being at a higher redshift.
I band Arp 297 from Palomar, in greyscale.
I band of bigger galaxy in Arp 297 from Palomar, in color.
I band of smaller galaxy in Arp 297 from Palomar, in color.
Arp 305. Notice the blue tidal debris
between the two galaxies.
