TL;DR
This paper reviews the equations used in stellar interior models to account for axial rotation, discusses underlying assumptions, and explores the potential significance of rotation effects at low metallicity.
Contribution
It provides a comprehensive overview of the current equations for stellar rotation and highlights the possible importance of rotation effects in low-metallicity stars.
Findings
Rotation effects may be crucial at low metallicity.
Current models rely on specific hypotheses about rotation.
The paper clarifies the equations and assumptions used in stellar rotation modeling.
Abstract
In these lecture notes, we present the equations presently used in stellar interior models in order to compute the effects of axial rotation. We discuss the hypotheses made. We suggest that the effects of rotation might play a key role at low metallicity.
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