Astrophysics II
Accretion disks are structures formed by the gravitational attraction of a massive object, where matter spirals inward and accumulates around it. These disks are commonly found around black holes, neutron stars, and young stellar objects, playing a critical role in the growth and evolution of these celestial bodies. As material from the surrounding environment falls into the gravitational well, it forms a rotating disk that can heat up due to friction and release energy in various forms, such as X-rays or radiation.
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