UGC 1840 | |
---|---|
Observation data | |
Constellation | Andromeda |
Right ascension | 02h 23m 08.4268s |
Declination | +41° 22′ 20.031″ |
Redshift | 0.018096 |
Heliocentric radial velocity | 5,420 km/s |
Distance | 258.5 Mly (79.1 Mpc) |
Characteristics | |
Type | Peculiar |
Size | ~131,100 ly (40.20 kpc) (estimated) |
Notable features | Collisional ring galaxy |
Other designations | |
IRAS 02200+4108, 2MASX J02231142+4122047, Arp 145, MCG +07-06-002, PGC 9060 & 9062, CGCG 538-056, HFLLZOA F264, V Zw 229 |
UGC 1840, also 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] The earliest known reference to the pair of galaxies is in part 2 of the Morphological Catalogue of Galaxies, published in 1964, where it is listed as MCG +07-06-002.[2]
Made up of two galaxies, UGC 1840 NED01 (PGC 9060)[3] and UGC 1840 NED02 (PGC 9062),[4] the two galaxies had recently collided with each other[5] in which the elliptical galaxy has penetrated through the spiral galaxy's nucleus leaving a hole in its middle, thus forming a ring galaxy.[6][7] 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.[8][unreliable source?]
Both galaxies are listed as Arp 145 in the Atlas of Peculiar Galaxies which was created by Halton Arp.[9][10] They fall under the category of objects that have emanating material and both classified as galaxies that have ring systems.