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Explore the complex world of stellar outflows through this 40-minute lecture that delves into hydrodynamic simulations and multi-wavelength observations of cool, evolved stars. Discover how various structures like equatorial and bipolar outflows, cavities, clumps, arcs, shells, and spirals form in circumstellar environments. Learn about cutting-edge research combining detailed simulations with observational data to understand the physical processes driving stellar winds, outbursts, and explosions. Gain insights into specific astronomical phenomena including symbiotic binaries, bow shocks around runaway stars, and the mechanisms behind nova and interacting supernova explosions.
