Classical stellar evolution theories have undergone some drastic
changes in recent decades. New insights into the development of
stellar interiors were obtained from studying stars in various
stages of their lives, as well as with the help of fast computers,
which gave a boost to the branch of numerical modelling of
stellular structure and evolution. This book is divided into two
parts. The first part deals with the general aspects of stellular
structure and evolution including a chapter on numerical modelling.
The second part deals with specific evolutionary aspects of single
and binary stars with a variety of masses. The last chapter gives
several models of stars with specific masses. The book is intended
as an introduction for students, as well as a reference for
researchers.
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