Table of contents
Stellar Equilibrium With and Without Rotation
Physical Properties of Stellar Matter
Hydrodynamical Instabilities and Transport Processes
Acoustic and Gravity Waves. Helio- and Asteroseismology
Main-Sequence and Post-MS Evolution
About this book
Rotation is ubiquitous at each step of stellar evolution, from star formation to the final stages, and it affects the course of evolution, the timescales and nucleosynthesis. Stellar rotation is also an essential prerequisite for the occurrence of Gamma-Ray Bursts.
In this book the author thoroughly examines the basic mechanical and thermal effects of rotation, their influence on mass loss by stellar winds, the effects of differential rotation and its associated instabilities, the relation with magnetic fields and the evolution of the internal and surface rotation. Further, he discusses the numerous observational signatures of rotational effects obtained from spectroscopy and interferometric observations, as well as from chemical abundance determinations, helioseismology and asteroseismology, etc.
On an introductory level, this book presents in a didactical way the basic concepts of stellar structure and evolution in "track 1" chapters. The other more specialized chapters form an advanced course on the graduate level and will further serve as a valuable reference work for professional astrophysicists.
- DOI https://doi.org/10.1007/978-3-540-76949-1
- Copyright Information Springer Berlin Heidelberg 2009
- Publisher Name Springer, Berlin, Heidelberg
- eBook Packages Physics and Astronomy
- Print ISBN 978-3-540-76948-4
- Online ISBN 978-3-540-76949-1
- Series Print ISSN 0941-7834
- Buy this book on publisher's site