PGC 4035 (= IC 76 = PGC 143948)
PGC 4070 (= PGC 2800925)
A 15th-magnitude spiral galaxy (type S?) in Cetus (RA 01 08 52, Dec -15 25 19)
As noted there, sometimes confused with IC 80. In the same cluster of galaxies as IC 80 (probably Abell 166, but usually stated as Abell 151, as discussed at that entry). Based on recessional velocity of 16530 km/sec, about 740 million light years away (another measurement of 17450 km/sec puts it another 40 million light years further away, but either way, it is in the distance range for Abell 166). Given that and apparent size of 0.6 by 0.4 arcmin, about 130 thousand light years across. |
Above, a 1 arcmin wide closeup of PGC 4070
Below, a 4.5 arcmin region centered on IC 80, showing the location of PGC 4070
PGC 4071 (with PGC 4072 = IC 80 (pair also = PGC 3325365)
PGC 4072 (= PGC 138321; with PGC 4071 = IC 80 (pair also = PGC 3325365)
PGC 4079 (= IC 78)
PGC 4082 (= IC 79)
PGC 4103 (= IC 82)
PGC 4116 (= Arp 11)
A 14th-magnitude spiral galaxy (type SBb) in Pisces (RA 01 09 22, Dec +14 20 32)
Based on recessional velocity of 11520 km/sec, about 510 million light years away. Given that and apparent size of 1.7 by 0.6 arcmin, about 250 thousand light years across. |
Above, a 1.5 arcmin wide closeup of Arp 11
Below, a 12 arcmin wide region centered on the galaxy
PGC 4127 (= IC 81)
PGC 4182 (= IC 83)
PGC 4265 (= IC 84)
PGC 4455
A 16th-(b)magnitude dwarf galaxy (type Sd?) in Cetus (RA 01 14 21, Dec +00 55 02)
Commonly misidentified as IC 88, as noted at that location. Based on recessional velocity of 1130 km/sec, about 50 million light years away (although given the relatively small velocity, peculiar (non-Hubble redshift) velocities could considerably alter this result). Given that and apparent size of 0.6 by 0.25 arcmin, about 9 thousand light years across. |
Above, a 1 arcmin wide closeup of PGC 4455
Below, a 12 arcmin wide region centered on the galaxy |
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