IC 64
| IC 64 | |
|---|---|
 SDSS image of lenticular galaxy IC 64 | |
| Observation data (J2000 epoch) | |
| Constellation | Pisces |
| Right ascension | 00h 59m 24.4s |
| Declination | +27° 03′ 32.6″ |
| Redshift | 0.045932 |
| Heliocentric radial velocity | 13,738 km/s |
| Distance | 622 Mly (190.7 Mpc) |
| Apparent magnitude (V) | 0.16[citation needed] |
| Apparent magnitude (B) | 0.22[citation needed] |
| Characteristics | |
| Type | E/S0/ AGN |
| Size | 300,000 ly |
| Apparent size (V) | 1.3' x 1.1' |
| Other designations | |
| PGC 3550, UGC 613, MCG+04-03-031, CGCG 480-030, NVSS J005924+270332, LEDA 3550, NSA 128233, GB6 B0056+2647, RX J005924.5+270333 | |
IC 64 is a massive lenticular galaxy located 622 million light-years away in the Pisces constellation.[1][2][3] IC 64 has a diameter of 300,000 light-years, making it, three times bigger than the Milky Way and one of the largest galaxies observed.[4] IC 64 was discovered by French astronomer Stephane Javelle on 5 December 1893.[4] It has an active galactic nucleus,[1][5] and is an emission line galaxy.[6][7]
References
[edit]- ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-19.
- ^ "IC 64 - Lenticular Galaxy in Pisces | TheSkyLive.com". theskylive.com. Retrieved 2024-04-19.
- ^ Astronomy, Go. "IC 64 | galaxy in Pisces | IC List | GO ASTRONOMY". Go-Astronomy.com. Retrieved 2024-04-19.
- ^ a b "Index Catalog Objects: IC 50 - 99". cseligman.com. Retrieved 2024-04-19.
- ^ Zaw, Ingyin; Chen, Yan-Ping; Farrar, Glennys R. (2019-02-01). "A Uniformly Selected, All-sky, Optical AGN Catalog". The Astrophysical Journal. 872 (2): 134. arXiv:1902.03799. Bibcode:2019ApJ...872..134Z. doi:10.3847/1538-4357/aaffaf. ISSN 0004-637X.
- ^ Caccianiga, A.; Maccacaro, T.; Wolter, A.; Della Ceca, R.; Gioia, I. M. (2000-06-01). "Emission line AGNs from the REX survey. Results from optical spectroscopy". Astronomy and Astrophysics Supplement Series. 144: 247–269. arXiv:astro-ph/0004038. Bibcode:2000A&AS..144..247C. doi:10.1051/aas:2000344. ISSN 0365-0138.
- ^ Marziani, P.; D’Onofrio, M.; Bettoni, D.; Poggianti, B. M.; Moretti, A.; Fasano, G.; Fritz, J.; Cava, A.; Varela, J.; Omizzolo, A. (2017-03-01). "Emission line galaxies and active galactic nuclei in WINGS clusters". Astronomy & Astrophysics. 599: A83. arXiv:1608.07924. Bibcode:2017A&A...599A..83M. doi:10.1051/0004-6361/201628941. ISSN 0004-6361.
