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Explore the fascinating lecture on the end state of stars presented by G Srinivasan from the Raman Research Institute (RRI). This 1 hour and 20 minute presentation delves into the ultimate fate of stellar objects, examining what happens when stars exhaust their nuclear fuel and reach the final stages of their evolution. Learn about phenomena such as white dwarfs, neutron stars, and black holes as the fundamental end states of different stellar masses.
