Evolution of Massive Population III Stars

Sung-Chul Yoon

doi:10.14311/APP.2014.01.0066

Evolution of Massive Population III Stars

Authors

Sung-Chul Yoon Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul, 151-742

DOI:

https://doi.org/10.14311/APP.2014.01.0066

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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Published

2014-12-04

How to Cite

Yoon, S.-C. (2014). Evolution of Massive Population III Stars. Acta Polytechnica CTU Proceedings, 1(1), 66–70. https://doi.org/10.14311/APP.2014.01.0066