This book presents the fundamental concepts of the theory,
illustrated by numerous examples of astrophysical applications.
Classical concepts are combined with new developments and the
authors demarcate what is well established and what is still under
debate. To book illustrates how apparently complicated phenomena
can be addressed and understood using well-known physical
principles and equations within appropriate approximations and
simplifications. For this purpose, a number of astrophysical
examples are considered in greater detail than what is normally
presented in a regular textbook. In particular, a number of
nonlinear self-consistent models are considered, which is motivated
by the latest observational data and modern theory.
General
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