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How does fluid mechanics apply to galaxy dynamics?

Astrophysical fluid dynamics is a branch of modern astronomy that applies fluid mechanics to understand the motion of matter in outer space. It uses fundamental mathematical frameworks like the Navier-Stokes equations, continuity equations, and Euler's equations to model cosmic phenomena. Key applications range from explaining the behavior of stars and interstellar nebulae to examining accretion disks, astrophysical jets, and the fluid dynamics of entire galaxies.

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