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X-Ray Flare From NGC 3783’s Black Hole Triggers Ultrafast 60,000 km/s Winds

Researchers attribute the outflow to a sudden magnetic “unwinding” akin to a solar coronal mass ejection.

Overview

  • ESA’s XMM-Newton and JAXA’s XRISM captured a brief X-ray burst followed by powerful outflows in the active galaxy NGC 3783.
  • High-resolution spectroscopy from XRISM’s Resolve and XMM-Newton’s EPIC measured wind speeds near 60,000 km/s, about one-fifth the speed of light.
  • The winds formed within roughly a day of the flare, providing the first direct observation of such rapid onset in an active galactic nucleus.
  • The central black hole is estimated at about 30 million solar masses and drives a bright, energetic nucleus that emits jets and winds.
  • The findings, published in Astronomy and Astrophysics, reflect a joint ESAJAXANASA effort and show how complementary instruments can decode fast AGN outflows.