The impact of rotation on the properties of low-mass stars at different evolutionary stages is first described by discussing the properties of stellar models computed with shellular rotation. The observational constraints that are currently available to progress in our understanding of these dynamical processes are then presented, with a peculiar focus on asteroseismic measurements of red-giant stars.
CITATION STYLE
Eggenberger, P. (2015). Effects of rotation on stellar evolution and asteroseismology of red giants. In Astrophysics and Space Science Proceedings (Vol. 39, pp. 33–41). Kluwer Academic Publishers. https://doi.org/10.1007/978-3-319-10993-0_4
Mendeley helps you to discover research relevant for your work.