Led by Andrea Botteon of Italy’s National Institute for Astrophysics, the team utilized NASA’s Chandra X-ray Observatory and the German eROSITA telescope to pierce through the galactic plane. Their findings, published in Astronomy & Astrophysics, reveal a two-stage evolutionary process. Initially, a central supermassive black hole ejected high-speed clouds of charged particles and magnetic fields, creating a radio-bright trail that eventually began to fade as the particles lost energy.
The structure regained its brilliance following a violent collision between two massive galaxy clusters. This merger generated shock waves—akin to sonic booms from supersonic jets—that re-energized the decaying clouds. By isolating the hot gas emissions within the cluster, researchers determined the collision occurred along a horizontal axis several hundred million years ago. The two clusters are currently receding from one another, leaving behind the distinctive, twisted signature that caught the attention of astronomers.





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