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New research reveals how this "supercritical" feeding frenzy spins up the star and builds towering columns of X-ray light.

  • Writer: Sandeep K S
    Sandeep K S
  • Dec 14, 2025
  • 1 min read
Illustration explaining the dramatic variability of neutron star NGC 7793 P13, featuring two distinct phases. In the Faint Phase (2021), the star exhibits low X-ray luminosity and slower rotation acceleration. In the Bright Phase (2022-2024), increased X-ray brightness and doubled rotation acceleration are observed, linked to supercritical accretion processes.
Illustration explaining the dramatic variability of neutron star NGC 7793 P13, featuring two distinct phases. In the Faint Phase (2021), the star exhibits low X-ray luminosity and slower rotation acceleration. In the Bright Phase (2022-2024), increased X-ray brightness and doubled rotation acceleration are observed, linked to supercritical accretion processes.

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