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Stellar Structure and Evolution (Astronomy and Astrophysics Library)
 
 
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Stellar Structure and Evolution (Astronomy and Astrophysics Library) [Hardcover]

Rudolf Kippenhahn (Author), A. Weigert (Author)
4.0 out of 5 stars  See all reviews (4 customer reviews)


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Kindle Edition $67.64  
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Book Description

0387502114 978-0387502113 November 1990
This text gives a complete and 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. The authors have written a unique text based on their own pioneering work in stellar modeling. Since its publication, this textbook has come to be considered a classic by readers and teachers in astrophysics. This study edition is meant for graduate students in astronomy and physics alike.
--This text refers to the Paperback edition.


Editorial Reviews

Review

"Kippenhahn and Weigert's work compares favorably with the few similar works, many of which are now out of date. It is superior to some others eschewing elegance of mathematical analysis in favor of a comprehensive understanding of the observed and deduced properties of stars, from their initial formation to their final collapse." -- Choice

"Will clearly be the standard text in the subject." -- N.H. Baker, Columbia University --This text refers to the Paperback edition.

Product Details

  • Hardcover: 468 pages
  • Publisher: Springer-Verlag (November 1990)
  • Language: English
  • ISBN-10: 0387502114
  • ISBN-13: 978-0387502113
  • Product Dimensions: 9 x 6 x 0.4 inches
  • Shipping Weight: 10.4 ounces
  • Average Customer Review: 4.0 out of 5 stars  See all reviews (4 customer reviews)
  • Amazon Best Sellers Rank: #3,518,052 in Books (See Top 100 in Books)

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Customer Reviews

4 Reviews
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Average Customer Review
4.0 out of 5 stars (4 customer reviews)
 
 
 
 
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4 of 4 people found the following review helpful:
4.0 out of 5 stars Among astro texts..., November 16, 2008
By 
Ashley (California, USA) - See all my reviews
This text supports most every assertion with lengthy and invaluable derivations that are useful in ensuring that students understand the material. The topics are covered with exceptional depth, and the explanations are unusually readable. Compared with other astrophysics textbooks marketed to a similar audience, _Stellar Structure and Evolution_ is the sort of resource that will follow me through future courses, and although it was only recommended (rather than required) for my current class, I'm extremely glad I decided to purchase it.
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5 of 7 people found the following review helpful:
4.0 out of 5 stars A star's lifetime, July 29, 2004
What happens in the lifetime of a star? This basically is the subject of the book. It describes from basic physical principles where ever possible how a star is formed and how it burns. Kippenhahn shows how inside a star, the gravitational pressure is necessarily balanced by the outgoing radiation and matter pressure.

We see the cycle of how a star burns its hydrogen, synthesising helium in the process. Then, how heavier elements are formed. Finally, whether a star novas or not, depending on its mass.

The Hertzsprung-Russell diagram is shown as a concise way to describe the lifecycle trajectory of a star, over billions of years.

Well suited for physics students.
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1 of 3 people found the following review helpful:
5.0 out of 5 stars very nice book, May 9, 2008
By 
Zanata Christian (Lovadina, Treviso, Italy) - See all my reviews
(REAL NAME)   
very nice book, clear and good written.

it permits me to pass the university exam, because the professor use it for his lessons.

just to know that it italy this book costs over 150 euro!
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Inside This Book (learn more)
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Key Phrases - Statistically Improbable Phrases (SIPs): (learn more)
thermal adjustment time, central helium burning, central hydrogen burning, solar standard model, hydrogen shell source, helium shell source, pycnonuclear reactions, helium main sequence, stellar centre, homologous contraction, convective stars, neutrino losses, hydrogen main sequence, piston model, homologous changes, polytropic relation, given mass element, carbon flash, vibrational instability, time tff, deflagration front, convective core, vibrational stability, neighbouring solutions, envelope solutions
Key Phrases - Capitalized Phrases (CAPs): (learn more)
Los Alamos, Teff Fig
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