Galaxy cluster in constellation Canes Venatici
The Canes II Group or Canes Venatici II Group (CVn II Group) is a group of galaxies about 26.1 million light-years away from Earth. The group resides in the Local Supercluster.[1] The largest galaxy within the cluster is M106 (NGC 4258), which is a barred spiral galaxy.[2]
Galaxies in the Cluster
Canes II is directly behind Canes I, which makes it difficult to show which galaxy belongs in which cluster.[2] It is generally accepted that the following galaxies belong in Canes II;[2]
Name
|
Equatorial Coordinates
|
Declination
|
Blue Magnitude
|
Type
|
Angular Diameter arc.
|
Galaxy Diameter (Kly)
|
Recessional Velocity
|
Other Names
|
NGC 4096 |
12 06.0 |
+47 29 |
11.5 |
Barred Spiral-c |
6.5 |
55 |
770 |
None
|
NGC 4144 |
12 10.0 |
+46 27 |
12.2 |
Barred Spiral-c |
6.0 |
55 |
481 |
|
UGC 7267 |
12 15.4 |
+51 22 |
15.3 |
Spiral-d |
1.7 |
15 |
660 |
|
UGC 7271 |
12 15.6 |
+43 26 |
15.5 |
Spiral-c |
1.6 |
15 |
772 |
|
UGC 7298 |
12 16.5 |
+52 13 |
17 |
Irregular |
1.3 |
10 |
354 |
|
UGC 7320 |
12 17.5 |
+44 29 |
Unknown |
Spiral-d |
.9 |
10 |
740 |
|
NGC 4242 |
12 17.5 |
+45 37 |
11.7 |
Barred Spiral-m |
4.8 |
40 |
733 |
|
NGC 4248 |
12 17.8 |
+47 25 |
13.4 |
Barred Spiral-b |
2.4 |
20 |
693 |
|
M106 |
12 19.0 |
+47 18 |
9.1 |
Barred Spiral-b |
17.0 |
150 |
656 |
NGC 4258
|
UGC 7356 |
12 19.2 |
+47 05 |
15.8 |
Irregular |
.9 |
10 |
480 |
|
NGC 4288 |
12 20.6 |
+46 18 |
13.4 |
Barred Spiral-c |
2.2 |
20 |
746 |
|
UGC 7408 |
12 21.3 |
+45 49 |
13.4 |
Irregular |
2.6 |
20 |
675 |
DDO 120
|
UGC 7599 |
12 28.5 |
+37 14 |
14.9 |
Spiral-m |
1.9 |
15 |
527 |
DDO 127
|
UGC 7608 |
12 28.8 |
+43 14 |
13.7 |
Irregular |
3.5 |
30 |
760 |
DDO 129
|
NGC 4460 |
12 28.8 |
+44 52 |
12.8 |
Spiral-0 |
4.1 |
35 |
711 |
|
UGC 7639 |
12 29.9 |
+47 32 |
14.5 |
Irregular |
2.4 |
20 |
585 |
|
KK151 |
12 30.4 |
+42 54 |
16.5 |
Spiral-c |
1.1 |
10 |
660 |
PGC 41314
|
NGC 4485 |
12 30.5 |
+41 42 |
12.5 |
Irregular |
2.4 |
20 |
725 |
|
NGC 4490 |
12 30.6 |
+41 38 |
10.6 |
Barred Spiral-c |
6.3 |
55 |
809 |
|
UGC 7678 |
12 32.0 |
+39 50 |
16.1 |
Barred Spiral |
0.9 |
10 |
921 |
|
UGC 7690 |
12 32.4 |
+42 42 |
13.4 |
Irregular |
1.6 |
15 |
762 |
|
UGC 7699 |
12 32.8 |
+37 37 |
13.6 |
Barred Spiral-c |
3.8 |
35 |
743 |
|
UGC 7719 |
12 34.0 |
+39 01 |
15.3 |
Spiral-d |
1.9 |
15 |
920 |
|
UGC 7751 |
12 35.1 |
+41 03 |
17.6 |
Irregular |
0.7 |
5 |
835 |
|
UGC 7774 |
12 36.4 |
+40 00 |
15.0 |
Spiral-c |
3.0 |
25 |
758 |
|
UGC 7827 |
12 39.7 |
+44 51 |
17? |
Irregular |
1.2 |
10 |
765 |
|
NGC 4618 |
12 41.6 |
+41 09 |
11.4 |
Barred Spiral-d |
4.4 |
40 |
771 |
|
NGC 4625 |
12 41.9 |
+41 16 |
13.1 |
Barred Spiral-m |
2.1 |
20 |
837 |
|
UGC 7949 |
12 47.0 |
+36 29 |
15.1 |
Irregular |
1.9 |
15 |
578 |
DDO 147
|
NGC 4707 |
12 48.4 |
+51 10 |
13.4 |
Spiral-m |
2.2 |
20 |
646 |
|
References
- ^ G. De Vaucouleurs, 1975. Nearby Groups of Galaxies, ch. 5. the nearer groups within 10 megaparsecs. Published in "Galaxies and the Universe," ed. by A. Sandage, M. Sandage and J. Kristian
- ^ a b c "The Canes II Group". Atlas of the Universe. 2003. Retrieved 2009-08-06.
See also