Magnetohydrodynamics
Accretion disks are structures formed by diffuse material in orbital motion around a central massive body, often found in astrophysical contexts such as stars, black holes, and neutron stars. These disks play a crucial role in the transfer of angular momentum and energy, influencing the growth of celestial objects and the dynamics of space plasmas. The interactions within these disks can lead to phenomena like jet formation and instabilities that significantly affect their evolution.
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