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Explore the collision and merger products of stars through magnetohydrodynamic (MHD) simulations in this one-hour conference presentation. Examine how stellar collisions and mergers produce different outcomes by analyzing the complex interplay between magnetic fields, fluid dynamics, and stellar material during these extreme astrophysical events. Learn about the computational methods used to model these phenomena and discover how MHD effects influence the final products of stellar interactions. Gain insights into the physical processes that govern stellar collisions versus mergers, including the role of magnetic fields in shaping the resulting stellar remnants and their observable characteristics. Understand the implications of these findings for stellar evolution theory and observational astronomy.
