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Stellar Structure and Evolution of Massive Rotating Single Stars

Published online by Cambridge University Press:  29 August 2024

R. Hirschi Open the ORCID record for R. Hirschi [Opens in a new window] ,
E. Kaiser ,
P. Eggenberger ,
S. Ekström ,
C. Georgy ,
A. Maeder  and
G. Meynet
R. Hirschi*
Affiliation:
Astrophysics Group, Lennard-Jones Laboratories, Keele University, Keele ST5 5BG, UK Kavli IPMU (WPI), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa 277-8583, Japan
E. Kaiser
Affiliation:
Astrophysics Group, Lennard-Jones Laboratories, Keele University, Keele ST5 5BG, UK
P. Eggenberger
Affiliation:
Geneva Observatory, Geneva University, CH-1290 Sauverny, Switzerland
S. Ekström
Affiliation:
Geneva Observatory, Geneva University, CH-1290 Sauverny, Switzerland
C. Georgy
Affiliation:
Geneva Observatory, Geneva University, CH-1290 Sauverny, Switzerland
A. Maeder
Affiliation:
Geneva Observatory, Geneva University, CH-1290 Sauverny, Switzerland
G. Meynet
Affiliation:
Geneva Observatory, Geneva University, CH-1290 Sauverny, Switzerland
*
email: [email protected]
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Abstract

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Rotation plays an important role in the structure and evolution of massive stars. It leads to deviation from spherical symmetry for very fast rotating stars, mixing in otherwise unmixed radiative regions and generally increased mass loss. In addition, magnetic fields interact with rotation and lead to significant transport of angular momentum. In this article, we review the various rotational and magnetic instabilities present in massive stars and their implementation in one-dimensional stellar evolution codes. We then focus on their impact on the evolution of single rotating stars. Finally, we compare rotating models to observations and discuss ways to disentangle between various uncertainties.

Keywords

rotation - hydrodynamics - magnetism - stars: evolutioninteriorsmassive
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S361: Massive Stars Near and Far , May 2022 , pp. 343 - 352
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Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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