Astrophysical Fluid Dynamics studies the behavior of fluids in astrophysical environments such as stars, galaxies, accretion disks, and interstellar gas clouds. In these systems, gravity, radiation, magnetic fields, and compressibility strongly influence fluid motion. Astrophysical flows often involve extreme temperatures, densities, and velocities. This field explains processes such as star formation, supernova explosions, and galaxy evolution. Astrophysical fluid dynamics combines hydrodynamics, magnetohydrodynamics, and radiation transport. Observations from telescopes and space missions guide theoretical models and simulations. Understanding astrophysical fluid behavior is essential for interpreting cosmic phenomena and the large-scale structure of the universe. This field bridges classical fluid mechanics and modern astrophysics.
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Yarub Al Douri, European Academy of Sciences, Belgium
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