NGC 2325 is a radio galaxy, i.e. it has giant regions of radio emission extending well beyond its visible structure. It also has an active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
Galaxy group
NGC 2325 is a member of a galaxy group known as [CHM2007] HDC 421. The group contains at least eight galaxies, including IC 456, ESO 427-22, MCG-05-17-006, MCG-05-17-004, MCG-05-17-008, and two others.
SN 2010ih (TypeIa, mag. 13.3) was discovered by The CHilean Automatic Supernova sEarch (CHASE) on 29 September 2010. A prediscovery image taken on 16 September showed it at magnitude 12.8, making it the brightest supernova of 2010.
↑Charlot, P.; Jacobs, C. S.; Gordon, D.; Lambert, S.; De Witt, A.; Böhm, J.; Fey, A. L.; Heinkelmann, R.; Skurikhina, E.; Titov, O.; Arias, E. F.; Bolotin, S.; Bourda, G.; Ma, C.; Malkin, Z.; Nothnagel, A.; Mayer, D.; MacMillan, D. S.; Nilsson, T.; Gaume, R. (2020). "The third realization of the International Celestial Reference Frame by very long baseline interferometry". Astronomy and Astrophysics. 644: A159. arXiv:2010.13625. Bibcode:2020A&A...644A.159C. doi:10.1051/0004-6361/202038368.
↑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.