IC 4271 | |
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![]() IC 4271 captured by Hubble | |
Observation data (J2000 epoch) | |
Constellation | Canes Venatici |
Right ascension | 13h 29m 21.40s |
Declination | +37d 24m 42.0s |
Redshift | 0.057000 |
Heliocentric radial velocity | 16,625 km/s |
Distance | 800 Mly (245.3 Mpc) |
Apparent magnitude (V) | 15 (15.3) |
Apparent magnitude (B) | 15.8 (16.3) |
Surface brightness | 13.3 (12.5) |
Characteristics | |
Type | SBab? pec + Sc? |
Size | 157,000 ly (48.16 kpc) |
Apparent size (V) | 0.8' x 0.5' |
Other designations | |
PGC 47334, Arp 40, NVSS J132921+372447, MCG +06-30-15, Z 190-12, VV 355 |
IC 4271 is a spiral galaxy located some 800 million light-years away in the Canes Venatici constellation. [1] It is 157,000 light-years in diameter. [2] IC 4271 was first located on July 10, 1896, by Stephane Javelle, a French astronomer. [2] It hosts a Seyfert type 2 nucleus, containing an acceleration disc around its supermassive black hole which releases large amounts of radiation, hence its bright appearance. [3] [4] IC 4271 appears to be interacting with its smaller neighboring galaxy, PGC 3096774. [2] [5] [6]
Both galaxies form Arp 40. [7] [8] In the Atlas of Peculiar Galaxies created by Halton Arp, they fall under spiral galaxies that have companions with low-surface-brightness.