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Trapped Jets in Massive Stars Revealed as Source of Fast X-Ray Transients

Frequent Einstein Probe detections followed by Rubin Observatory surveys will allow researchers to probe how jets fail to break through collapsing stars

Overview

  • Detailed observations of EP 250108a and its associated supernova SN 2025kg confirm that fast X-ray transients originate from jets that stall inside the outer layers of collapsing massive stars.
  • Since its 2024 launch, the Einstein Probe has detected FXTs several times per month, vastly outpacing the roughly annual gamma-ray burst rate and suggesting failed-jet explosions are common.
  • Rapid multi-wavelength follow-ups with the International Gemini Observatory’s FLAMINGOS-2 and GMOS instruments, along with SOAR Telescope data, tracked the evolving X-ray, optical and infrared signals of the event.
  • Spectroscopic analysis identifies EP 250108a/SN 2025kg as a Type Ic broad-lined supernova from a progenitor star of about 15–30 solar masses.
  • Researchers are gearing up to exploit the upcoming Vera C. Rubin Observatory LSST to expand transient surveys and deepen understanding of jet-failure mechanisms.