NGC 5614
Appearance
NGC 5614 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Boötes |
Right ascension | 14h 24m 07.591s[1] |
Declination | +34° 51′ 32.02″[1] |
Redshift | 0.012970[2] (3,891 km/s ) |
Distance | 194.9 Mly (59.76 Mpc)[3] |
Apparent magnitude (V) | 12.6[4] |
Characteristics | |
Type | SA(r)ab pec[4] |
Apparent size (V) | 1.567′ × 1.410′[1] |
Notable features | NGC 5615 superimposed, plume, paired with NGC 5613. |
Other designations | |
2MASX J14240759+3451320, CGCG 192.014, GC 3880, h 1804, H 2.420, H II-420, IRAS 14220+3505, ISOSS J14240+3451, MCG+06-32-022, PGC 51439, UGC 9226, UZC J142407.6+345134, VV 77a, LEDA 51439, Z 192-14, Z 1422.0+3505 |
NGC 5614 is a spiral galaxy in the constellation Boötes. It is the primary member of the Arp 178 triplet of interacting galaxies with NGC 5613 and NGC 5615.
References
- ^ a b c Skrutskie, M. F.; et al. (February 2006), "The Two Micron All Sky Survey (2MASS)", The Astronomical Journal, 131 (2): 1163–1183, Bibcode:2006AJ....131.1163S, doi:10.1086/498708.
- ^ Kochanek, C. S.; et al. (October 2001), "The K-Band Galaxy Luminosity Function", The Astrophysical Journal, 560 (2): 566–579, arXiv:astro-ph/0011456, Bibcode:2001ApJ...560..566K, doi:10.1086/322488.
- ^ Crook, Aidan C.; et al. (February 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.
- ^ a b "NED results for object NGC 5614", NASA/IPAC Extragalactic Database, NASA, retrieved 2015-10-29.
External links
- http://seds.org
- Image NGC 5614
- Distance
- SIMBAD data
- NGC 5614 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images