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Lecture 7 Evolution of Massive Stars on the Main Sequence and During Helium Burning - Basics

Lecture 7 Evolution of Massive Stars on the Main Sequence and During Helium Burning - Basics. Key Physics and Issues. Evolution in HR diagram Nucleosynthesis Surface abundances Presupernova structure Supernova properties Remnant properties Rotation and B-field of pulsars.

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Lecture 7 Evolution of Massive Stars on the Main Sequence and During Helium Burning - Basics