This volume is devoted to one of the fascinating things about
stars: how they evolve as they age. This evolution is different for
stars of different masses. How stars end their lives when their
supply of energy is exhausted also depends on their masses.
Interestingly, astronomers conjectured about the ultimate fate of
the stars even before the details of their evolution became clear.
Part I of this book gives an account of the remarkable predictions
made during the 1920s and 1930s concerning the ultimate fate of
stars. Since much of this development hinged on quantum physics
that emerged during this time, a detailed introduction to the
relevant physics is included in the book. Part II is a summary of
the life history of stars. This discussion is divided into three
parts: low-mass stars, like our Sun, intermediate-mass stars, and
massive stars. Many of the concepts of contemporary astrophysics
were built on the foundation erected by Subrahmanyan Chandrasekhar
in the 1930s. This book, written during his birth centenary,
includes a brief biographical sketch of the brilliant scientist,
which readers will find fascinating.
Reading this book will get young students excited about the
presently unfolding revolution in astronomy and the challenges that
await them in the world of physics, engineering and technology.
General readers will also find the book appealing for its highly
accessible narrative of the physics of stars.
This book is a companion volume of What are the Stars? by the
same author.
""I know of no other book on the evolution of stars of a similar
scope and breadth that is so accessible for undergraduate
students.""
E P J van den Heuvel
Professor of Astrophysics
Winner of the Spinoza and Descartes PrizesUniversity of
Amsterdam, The Netherlands
"
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