Astronomers from South Africa and India have analyzed archival data from the Chandra X-ray Observatory and Giant Metrewave Radio Telescope (GMRT) regarding a nearby small galaxy group known as IC 1262. Results of the new study, presented April 14 on the preprint server arXiv, provide more insights into metal enrichment of IC 1,262, which could help us better understand the nature of this group.
IC 1,262 is a rich galaxy group located at a redshift of 0.032, named after its brightest cluster galaxy (BCG). It exhibits complex substructures in its hot gas that include ripples, prominent sharp discontinuities (cold fronts) extending in both the east and west directions, a large-scale radio jet, recurrent active galactic nucleus (AGN) activity, and X-ray cavities filled with radio emission.
Recently, a group of astronomers led by Satish Shripati Sonkamble of the North-West University in South Africa has explored the IC 1,262 group in detail, focusing on metal transport via radio jet, sloshing cold fronts, and shock front. In general, it is assumed that cold fronts, gas sloshing, and AGN activity are responsible for metal enrichment in the intracluster medium (ICM) and intragroup medium (IGrM).









