| 752-4-52-929-734 | 151.382,0.071 | NED | SDSS |
Sextans C is a globular cluster, although it is also listed sometimes
(incorrectly) as a dwarf galaxy (UGC 05439).
|
| 756-3-756-818-816 | 229.013,-0.123 | NED | SDSS |
Globular cluster Palomar 5, a loose cluster of stars located in the halo of the
Milky Way.
|
| 756-2-484-695-949 | 188.283,-0.534 | NED | SDSS |
UGCA 285, an ultra low surface brightness galaxy. Galaxies come
in a variety of sizes and luminosities; this galaxy is barely detected
even with the highly sensitive Sloan Survey camera.
|
| 752-5-273-1141-250 | 184.483,0.436 | NED | SDSS |
UGC 07332, a nearby, blue, low surface brightness galaxy.
|
| 752-2-16-1259-1726 | 146.03,-0.658 | NED | SDSS |
UGC 05205, and its companion. These two galaxies are very
young, as indicated by their very blue colors. They mostly
consist of diffuse gas and a few clumps, the disk and bulge
have not formed yet.
|
| 125-6-140-1158-121 | 9.895,0.86 | NED | SDSS |
A nearby group of galaxies around NGC 0201. Galaxy groups
typically have about 10-20 members.
|
| 756-2-654-1184-1284 | 213.785,-0.4934 | NED | SDSS |
VIII Zw 388, a picturesque group of galaxies, discovered and
catalogued by the legendary Fritz Zwicky.
|
| 94-4-141-276-858 | 355.918,0.311 | NED | SDSS |
A clustering of galaxies at moderate redshift. One of the goals of the
Sloan Survey is to characterize the amount of clustering and to provide
clues as to how such clustering arose in the early universe.
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