| UGC 1840 | |
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Hubble Space Telescope image of UGC 1840
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| Observation data | |
| Constellation | Andromeda |
| Right ascension | 35.79 degrees |
| Declination | 41.36 degrees |
| Redshift | 0.018096 |
| Heliocentric radial velocity | 5,420 km/s |
| Distance | 258.5 Mly (79.1 Mpc) |
| Characteristics | |
| Type | PECULR |
| Notable features | Collisional ring galaxy |
| Other designations | |
| Arp 145, IRAS 02200+4108, PGC 9062, PGC 9060, MCG+07-06-002, UGC 1840, Z 538-56, HFLLZOA F264, V Zw 229, 2MASX J02231142+4122047 | |
UGC 1840 known as Arp 145, are a pair of interacting galaxies located 250 million light-years away from the Solar System in the Andromeda constellation.[1] Made up of two galaxies, UGC 1840 NED01 (PGC 9060)[2] and UGC 1840 NED02 (PGC 9062),[3] the two galaxies had recently collided with each other[4] in which the elliptical galaxy has penetrated through the spiral galaxy's nucleus leaving a hole in its middle, thus forming a ring galaxy.[5][6] With a diameter of 1.3 arc minutes, close to 100,000 thousand light-years, they are roughly the same size as the Milky Way.[7][unreliable source?]
Both galaxies are included in Atlas of Peculiar Galaxies which was created by Halton Arp.[8][unreliable source?] They fall under the category of objects that have emanating material and both classified as galaxies that have ring systems.
{{cite web}}: External link in |last=|
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