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Irregular galaxy in the constellation Canes Venatici
IC 883 is classified a luminous infrared galaxy (LIRG). It is a recent merger given that the galaxy has one single nucleus and two tidal tails. The molecular gas measured in IC 883 is estimated 4 x 10 MΘ. It is known to show a radio jet originating from its nucleus travelling at a subluminal motion of 0.6-1 c.
Two supernovae have been observed in IC 883: SN 2010cu (type II, mag. 17.7), and SN 2011hi (type II, mag. 17.9). When observed in near-infrared or optical wavelengths, they are the nearest supernovae found to the nucleus of an LIRG.
Modica, F.; Vavilkin, T.; Evans, A. S.; Kim, D. C.; Mazzarella, J. M.; Iwasawa, K.; Petric, A.; Howell, J. H.; Surace, J. A. (2011-11-14). "Multi-Wavelength Goals Observations of Star Formation and Active Galactic Nucleus Activity in the Luminous Infrared Galaxy Ic 883". The Astronomical Journal. 143: 16. arXiv:1111.3293. doi:10.1088/0004-6256/143/1/16.
Kankare, E.; Mattila, S.; Ryder, S.; Vaisanen, P.; Alberdi, A.; Alonso-Herrero, A.; Colina, L.; Efstathiou, A.; Kotilainen, J. (2011-12-04). "Discovery of Two Supernovae in the Nuclear Regions of the Luminous Infrared Galaxy Ic 883". The Astrophysical Journal. 744 (2): L19. arXiv:1112.0777. doi:10.1088/2041-8205/744/2/L19.
Sinnott, R. W. (1988). NGC 2000.0: The Complete New General Catalogue and Index Catalogues of Nebulae and Star Clusters. Sky Publishing. ISBN978-0-933346-51-2.