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Gravitational Physics of Stellar and Galactic Systems (Cambridge Monographs on Mathematical Physics) [Hardcover]

William C. Saslaw (Author)


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Book Description

August 30, 1985 052123431X 978-0521234313 First Edition
This text describes the gravitational interactions and evolution of astronomical systems on all scales, from small groups of stars through galaxies and clusters of galaxies to the Universe itself. In a rapidly developing area of astronomy, it is the first comprehensive treatise on the subject to be published since the early 1960s. Concentrating on the basic physics, at a graduate student level, it also develops many astronomical applications in considerable detail. The book is self-contained. Most results are derived from preceding ones in a straightforward way. It is written to bring out the physical content behind the mathematical formulae, and contains a number of exercises and suggestions for research topics. Bibliographies with nearly 300 selected references provide gateways into the literature.

Editorial Reviews

Review

' ... the author achieves a ery nice balance between mathematics, physics and astronomy as well as between the reality and simplicity of the models discussed.' Classical and Quantum Gravity

' ... eminently readable. It is written throughout in an engaging style with a clear logical development ... All this adds up to a beautifully presented account ... it will be much appreciated by both practising astronomers and beginning graduate students in astronomy.' Times Higher Education Supplement

' ... a beautifully written text on stellar physics and on dynamics ... The author has produced a work of literature, indispensible to anyone working on studies of stellar and galactic systems.' New Scientist

Book Description

This text describes the gravitational interactions and evolution of astronomical systems on all scales, from small groups of stars through galaxies and clusters of galaxies to the Universe itself. It is written to bring out the physical content behind the mathematical formulae, and contains a number of exercises and suggestions for research topics.

Product Details

  • Hardcover: 512 pages
  • Publisher: Cambridge University Press; First Edition edition (August 30, 1985)
  • Language: English
  • ISBN-10: 052123431X
  • ISBN-13: 978-0521234313
  • Shipping Weight: 2.4 pounds
  • Amazon Best Sellers Rank: #10,384,152 in Books (See Top 100 in Books)

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Inside This Book (learn more)
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First Sentence:
The self-consistent motions of all the stars or galaxies in an isolated cluster are completely determined by their mutual gravitational forces, so long as each object can be treated as a point mass. Read the first page
Key Phrases - Statistically Improbable Phrases (SIPs): (learn more)
normal polytropes, gravitational phase transitions, orbit segregation, cosmic energy equation, loaded polytropes, third isolating integral, adiabatic decay, spherical stellar systems, high energy stars, accreting star, clustering efficiency, probe star, impulsive approximation, violent relaxation, gravitational thermodynamics, soft binaries, gravitating systems, stellar hydrodynamics, hard binaries, dense stellar systems, slow encounters, zero velocity curve, collisionless systems, mass segregation, mean square position
Key Phrases - Capitalized Phrases (CAPs): (learn more)
New York, Einstein-de Sitter, Alexander Pope, Bibliography Section, Dynamics of Stellar Systems
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