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Accretion disk: Revision history

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25 January 2026

  • curprev 21:2521:25, 25 January 2026 DanteWashere talk contribs 664 bytes +664 Created page with "'''Accretion disk''' is a rotating structure of gas, dust, or plasma formed by material falling toward a central massive object under gravity. It is associated with energy release through friction and heating as material spirals inward. Accretion disks are discussed in astrophysics, high-energy astronomy, and studies of compact objects. == Status == Accretion disks are inferred and observed around objects such as black holes, neutron stars, and young stars. Models desc..."
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