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Supermassive black holes exert greater influence on cosmic environments than previously thought

New astronomical research indicates that supermassive black holes exert a much more profound influence on their cosmic environments than previously understood. Using the XRISM X-ray astronomy satellite, researchers studying the quasar H1821+643 discovered that the energy from black hole winds is approximately 100 times more powerful than earlier calculations suggested. These winds extend roughly 300,000 light-years beyond galactic boundaries, transporting energy comparable to several billion supernova explosions.

Complementary studies of nine nearby galaxies suggest that actively growing black holes may actually contribute to star formation rather than merely preventing it. Observations from the VLT/MUSE instrument revealed that active galactic nuclei (AGN) are associated with star-forming rings, arcs, and energized gas cones. These findings highlight a complex feedback cycle where the injection and accretion of material are linked, allowing black holes to actively reshape the evolution of their host galaxies through high-speed outflows and shocks.

Entities

Center for Astrophysics | Harvard & Smithsonian · H1821+643 · XRISM