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IC 64

From Wikipedia, the free encyclopedia
Galaxy in the constellation Pisces
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
Size300,000 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 ]
  1. ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024年04月19日.
  2. ^ "IC 64 - Lenticular Galaxy in Pisces | TheSkyLive.com". theskylive.com. Retrieved 2024年04月19日.
  3. ^ Astronomy, Go. "IC 64 | galaxy in Pisces | IC List | GO ASTRONOMY". Go-Astronomy.com. Retrieved 2024年04月19日.
  4. ^ a b "Index Catalog Objects: IC 50 - 99". cseligman.com. Retrieved 2024年04月19日.
  5. ^ Zaw, Ingyin; Chen, Yan-Ping; Farrar, Glennys R. (2019年02月01日). "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.
  6. ^ Caccianiga, A.; Maccacaro, T.; Wolter, A.; Della Ceca, R.; Gioia, I. M. (2000年06月01日). "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.
  7. ^ Marziani, P.; D’Onofrio, M.; Bettoni, D.; Poggianti, B. M.; Moretti, A.; Fasano, G.; Fritz, J.; Cava, A.; Varela, J.; Omizzolo, A. (2017年03月01日). "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.
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