Evolution of Massive Population III Stars

Sung-Chul Yoon

Abstract


While the evolution of massive stars in the local Universe is dominated by mass-loss, the evolution of massive Population III stars should be dominated by rotation. An important effect of rotation is rotationally-induced chemical mixing that can dramatically change the stellar structure and the nucleosynthesis. This has significant consequences in the predicted explosion types of Population III stars.

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ISSN 2336-5382 (Online)
Published by the Czech Technical University in Prague