| NGC 4614 | |
|---|---|
 SDSS image of NGC 4614 | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 41m 31.46397s[1] |
| Declination | +26° 02′ 33.6235″[1] |
| Redshift | 0.01594[2] |
| Heliocentric radial velocity | 4741 km/s[2] |
| Distance | 234.9 Mly (72.03 Mpc)[3] |
| Apparent magnitude (B) | 14.2[2] |
| Characteristics | |
| Type | SB0/a[4] |
| Other designations | |
| UGC 7851, MCG +04-30-012, PGC 42573[2] | |
NGC 4614 is a barred lenticular galaxy in the New General Catalog. It is located in the constellation of Coma Berenices. It was discovered in 1864 by the German astronomer Heinrich d'Arrest with a 11.9 inch (11 inch) diameter lens type telescope.[5]
One supernova, SN 2018ata (type Ia, mag. 20), was discovered in NGC 4614 on 10 April 2018.[6]
- ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051.
- ^ a b c d "NGC 4614". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-12-12.
- ^ Crook, Aidan C.; Huchra, John P.; Martimbeau, Nathalie; Masters, Karen L.; Jarrett, Tom; Macri, Lucas M. (2007). "Groups of Galaxies in the Two Micron All Sky Redshift Survey". The Astrophysical Journal. 655 (2): 790–813. arXiv:astro-ph/0610732. Bibcode:2007ApJ...655..790C. doi:10.1086/510201. S2CID 11672751.
- ^ "Results for object NGC 4614 (NGC 4614)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2020-12-12.
- ^ "NGC 4614". sim-id. Retrieved 2020-07-26.
- ^ Transient Name Server entry for SN 2018ata. Retrieved 25 March 2023.