Galaxies and the Universe
An accretion disk is a structure formed by the gravitational attraction of a massive object, where matter spirals inwards due to angular momentum conservation. These disks are crucial in the formation of celestial bodies and play a key role in the growth and activity of quasars, as they provide a reservoir of gas and dust that can be drawn towards the central supermassive black hole. The material in an accretion disk gradually loses energy and angular momentum, allowing it to fall into the black hole, often resulting in high-energy emissions that can be observed as quasars.
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