IC 4271 is a spiral galaxy located some 800 million light-years away in the Canes Venatici constellation.[1] It is 130,000 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]
IC 4271 | |
---|---|
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? |
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 |
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.
References
edit- ^ "IC 4271 NED01 - Barred Spiral Galaxy in Canes Venatici | TheSkyLive.com". theskylive.com. Retrieved 2024-04-16.
- ^ a b c "Index Catalog Objects: IC 4250 - 4299". cseligman.com. Retrieved 2024-04-16.
- ^ Lazaro, Enrico de (2022-05-20). "Hubble Looks at Curious Pair of Spiral Galaxies | Sci.News". Sci.News: Breaking Science News. Retrieved 2024-04-16.
- ^ "IC 4271". simbad.cds.unistra.fr. Retrieved 2024-04-16.
- ^ "IC 4271 NED02 - Galaxy in Canes Venatici | TheSkyLive.com". theskylive.com. Retrieved 2024-04-16.
- ^ "Revised IC Data for IC 4271". spider.seds.org. Retrieved 2024-07-24.
- ^ "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2024-04-16.
- ^ "Halton Arp's Atlas of Peculiar Galaxies". cseligman.com. Retrieved 2024-04-16.