Linked from

The 61 pages that link to Accretion disk, each with the reason it gives.

• NGC 5548Related: Its hot inner regions produce much of the nucleus’s variable radiation.

• Sagittarius A*Related: Infalling gas near the black hole can heat and emit radiation.

• Young stellar objectRelated: Material in the disk can continue feeding the growing central star.

• Astronomical black holesRelated: Friction heats infalling gas, making some black holes detectable across the electromagnetic spectrum.

• Astrophysical electromagnetic fieldsRelated: Magnetic stresses can transport angular momentum and power outflows from accreting systems.

• Astrophysical X-ray sourceBroader topic: Friction and compression heat infalling matter until the disk radiates X-rays.

• BL LacertaeRelated: Its comparatively weak optical signatures distinguish this source from many other active nuclei.

• Black hole astronomyRelated: Its intense radiation makes feeding black holes observable.

• Gamma-ray burst progenitorsRelated: After collapse or merger, disk accretion can supply energy to the relativistic jet.

• Laboratory studies of space and astrophysical plasmasBroader topic: Experiments examine magnetic instabilities that may drive angular-momentum transport in disks.

• Rotating black holeRelated: Its inner edge and emitted radiation depend on the black hole’s spin.