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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.
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