Arp 273
Arp 273 |
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Observation data (J2000 epoch) |
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Right ascension |
02h 21m 28.703s[1] |
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Declination |
+39° 22′ 32.65″[1] |
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Distance |
300 million ly |
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Other designations |
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UGC 1810, LEDA 8961, VV 323, Z 523-28, APG 273, 2MASX J02212870+3922326, VV 323a, [HVG99b] 02184+3909, CGPG 0218.4+3909, MCG+06-06-023, ZW V 223, KPG 64a, UZC J022128.6+392231, Z 0218.4+3909. |
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Arp 273 is a group of interacting galaxies, lying 300 million light years away in the constellation Andromeda. It was first described in the Atlas of Peculiar Galaxies, compiled by Halton Arp in 1966.[2] The larger of the spiral galaxies, known as UGC 1810, is about five times more massive than the smaller galaxy.[3] It has a disc that is tidally distorted into a rose-like shape by the gravitational pull of the companion galaxy below it, known as UGC 1813. The smaller galaxy shows distinct signs of active star formation at its nucleus,[4] and "it is thought that the smaller galaxy has actually passed through the larger one."[5]
Other images
Arp 273 zoom sequence.
References
External links
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Wikimedia Commons has media related to Arp 273. |
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| UGC |
- UGC 1806
- UGC 1807
- UGC 1808
- UGC 1809
- UGC 1810
- UGC 1811
- UGC 1812
- UGC 1813
- UGC 1814
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| Arp | |
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