Overview
- XMM-Newton and XRISM saw a sharp X-ray flare in the spiral galaxy NGC 3783 followed by winds that formed within about a day.
- Material was expelled at roughly 60,000 km/s, close to one-fifth the speed of light.
- XRISM’s Resolve instrument measured the flare and wind properties while XMM-Newton monitored the event’s evolution and strength.
- The team reports the first confirmed near-instant onset of an AGN ultra-fast outflow linked to a flare, from a black hole of about 30 million solar masses.
- The results were published in Astronomy & Astrophysics and the authors call for further observations and modeling to test the magnetic mechanism and gauge its impact on galaxy evolution.