Stellar evolution is the process by which a star changes over the course of time, influenced by factors like mass, temperature, and chemical composition. It involves several stages, from the birth of a star in a molecular cloud to its ultimate fate as a white dwarf, neutron star, or black hole. Understanding this process is crucial in studying radiation hydrodynamics and scaled astrophysical experiments, as it provides insights into the physical processes that govern stellar behavior and lifecycle.
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