KnowraTidal disruption eventLinked fromLinked fromThe 14 pages that link to Tidal disruption event, each with the reason it gives.All 14Broader topic 4Related 6Narrower topic 1Compared with 3Accretion diskRelated: Debris from the disrupted star can circularize into a short-lived accretion disk.Active galactic nucleusCompared with: Unlike sustained nuclear activity, it can mark a brief episode of black-hole feeding.Tidal forceBroader topic: The black hole’s tidal force can exceed the star’s internal binding forces.Supermassive black holeRelated: Such events expose otherwise quiet black holes by briefly lighting up their surroundings.Roche limitNarrower topic: The same competition between tidal forces and self-gravity appears on much larger scales.Tidal interactionBroader topic: This is an extreme case in which tidal interaction overwhelms an object's self-gravity.Tidal strippingBroader topic: It is a dramatic stellar-scale case of complete or near-complete tidal destruction.Tidal disruptionBroader topic: It is the most luminous astronomical manifestation of tidal breakup.Accretion (astrophysics)Compared with: Disruption supplies debris for accretion rather than representing gradual body growth.PerihelionRelated: An extremely small perihelion distance can expose an orbiting star to destructive tidal forces.KilonovaCompared with: Both can be luminous transients, but tidal disruption events involve a star and massive black hole, not compact-binary ejecta.Nuclear star clusterRelated: Events in galactic nuclei can constrain the masses of otherwise hard-to-detect black holes.Intermediate-mass black holeRelated: A distinctive disruption flare can expose a black hole in the intermediate-mass range.Ultra-high-energy cosmic rayRelated: Some models associate its relativistic outflows with acceleration to ultra-high energies.