Astrophysical jets from supermassive black holes are awe-inspiring phenomena. These jets, made of ionized gas, extend for millions of parsecs, and can reach relativistic speeds. They can alter their galactic surroundings, affecting the gas inside the host galaxy, and beyond that into the host cluster, whey they can disrupt star formation.

SMBH only emit these jets when they're actively feeding. The material they feed on gathers in a super-heated accretion disk, but not all of it is consumed by the SMBH. Some of it is ejected by these jets, driven by the powerful magnetic fields in the accretion disk.

Despite understanding the overall picture, astrophysicists struggle to answer certain questions about the process. New research in The Astrophysical Journal Letters examined the link between accretion and jets. It's titled " Disk Truncation Triggers Relativistic Jet Launching of a Highly Accreting Supermassive Black Hole ," and the co-lead authors are Hirofumi Noda and Kazuhiro Hada.…