Polar-ring galaxy: Difference between revisions
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! Objects related to polar-ring galaxies | ! Objects related to polar-ring galaxies | ||
| [[ESO 79-G5]], [[NGC 235]], [[ESO 474-G11]], [[ESO 296-G11]], [[A 0153-3034]], [[AM 0310-252]], [[ESO 202-IG5]],[[ESO 305-G21]], [[AM 0529-442]], [[A 0618-3633]], [[ESO 16-G16]], [[UGC 4892]], [[NGC 3034]], [[UGC 5485]], [[NGC 3310]], [[NGC 3406]], [[A 1123-232]], [[NGC 3718]], [[NGC 3808]], [[ESO | | [[ESO 79-G5]], [[NGC 235]], [[ESO 474-G11]], [[ESO 296-G11]], [[A 0153-3034]], [[AM 0310-252]], [[ESO 202-IG5]],[[ESO 305-G21]], [[AM 0529-442]], [[A 0618-3633]], [[ESO 16-G16]], [[UGC 4892]], [[NGC 3034]], [[UGC 5485]], [[NGC 3310]], [[NGC 3406]], [[A 1123-232]], [[NGC 3718]], [[NGC 3808]], [[ESO 171 IG5]], [[UGC 7636]], [[NGC 4643]], [[NGC 4753]], [[AM 1257-222]], [[UGC 8387]], [[A 1356-2618]], [[PG 163+658]], [[NGC 6240]], [[A 1837-6317]], [[ESO 341-IG4]], [[ESO 286-IG19]], [[A 2102-2345]], [[A 2111-5509]], [[AM 2115-574]], [[NGC 7252]], [[A 2225-5838]], [[ESO 146-IG29]], [[A 2226-2459]], [[ESO 109-IG23]], [[ESO 239-IG2]], [[A 2246-4909]], [[NGC 7465]] | ||
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! Typical examples of polar-ring galaxies (Boz, Peanut and X galaxies) | ! Typical examples of polar-ring galaxies (Boz, Peanut and X galaxies) | ||
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[[Category:Galaxy morphological types]] | [[Category:Galaxy morphological types]] | ||
[[de:Polarring-Galaxie]] | [[de:Polarring-Galaxie]] | ||
Revision as of 09:32, 20 March 2007
A polar-ring galaxy is a relatively rare type of galaxy, with only around 100 examples known. The best known polar-ring galaxy is NGC 4650A. It is theorized that the structure of these galaxies result from the collision of two galaxies. The collision results in a structure composed of two rings of material rotating at an approximate right angle to each other.
Formation of polar-ring galaxies
It is important to understand that the collision occurs so slowly that even over a lifetime, the movement is almost imperceptible. Also important is that once what is left of the interacting galaxy has gone on after the collision, the remaining static galaxy does not simply stop moving. The stars in the galaxy will continue on their new paths until they are dispersed and it is no longer a galaxy. What one sees when they look at a polar-ring galaxy is a freeze-frame of a former galaxy spilling out around itself, its stars destined to disperse over many light-years.
List of polar-ring galaxies
References
- Hubblesite.org Retrieved January 2007