This long-awaited "second edition" of the classical textbook on
"Stellar Structure and Evolution" by Kippenhahn and Weigert is a
thoroughly revised version of the original text. Taking into
account modern observational constraints as well as additional
physical effects such as mass loss and diffusion, Achim Weiss and
Rudolf Kippenhahn have succeeded in bringing the book up to the
state-of-the-art with respect to both the presentation of stellar
physics and the presentation and interpretation of current
sophisticated stellar models. The well-received and proven
pedagogical approach of the first edition has been retained.
The book provides a comprehensive treatment of the physics of the
stellar interior and the underlying fundamental processes and
parameters. The models developed to explain the stability, dynamics
and evolution of the stars are presented and great care is taken to
detail the various stages in a star's life. Just as the first
edition, which remained a standard work for more than 20 years
after its first publication, the second edition will be of lasting
value not only for students but also for active researchers in
astronomy and astrophysics.
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