Model for the Quasi-Periodic Oscillations (QPO) — or ’heartbeat’ — where the inner part of the accretion disc is oscillating in size and shape, shown as a cross-section in the plane of the disc.
Credit: Dr. Chichuan Jin of the National Astronomical Observatories, Chinese Academy of Sciences
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Runaway black hole ’leaves behind’ massive streak of stars in its wake - See Hubble’s view