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商品の説明
内容説明
Binary systems of stars are as common as single stars. Stars evolve primarily by nuclear reactions in their interiors, but a star with a binary companion can also have its evolution influenced by the companion. Multiple star systems can exist stably for millions of years, but can ultimately become unstable as one star grows in radius until it engulfs another. This volume, first published in 2006, discusses the statistics of binary stars; the evolution of single stars; and several of the most important kinds of interaction between two (and even three or more) stars. Some of the interactions discussed are Roche-lobe overflow, tidal friction, gravitational radiation, magnetic activity driven by rapid rotation, stellar winds, magnetic braking and the influence of a distant third body on a close binary orbit. A series of mathematical appendices gives a concise but full account of the mathematics of these processes.
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The State of the Art as it Exists Today
2007/1/14
形式:ハードカバー
This book is aimed at the last year undergraduate student, graudade student or researchers. The reader is expected to be familiar with the terminology of stellar astrophysics (spectral types, magnitudes and like). Within that background the author presents an excellent introduction to binary and multiple stars.
The book begins with an interesting discussion on just what is a binary star. With the whole universe rotating about itself, a binary star is simply two stars that are closer than others. But in a dense star field 'closer' has to be closer than it does in a star desert where the orbits of binary stars may be on the order of centuries.
This is not a book for the amateur, the math is heavy duty, indeed the author moved to Livermore Labs to get closer to massive computing power. He has included a series of mathematical appendicies which give a concise but full account of the mathematics of the processes involved with star behavior.
The book begins with an interesting discussion on just what is a binary star. With the whole universe rotating about itself, a binary star is simply two stars that are closer than others. But in a dense star field 'closer' has to be closer than it does in a star desert where the orbits of binary stars may be on the order of centuries.
This is not a book for the amateur, the math is heavy duty, indeed the author moved to Livermore Labs to get closer to massive computing power. He has included a series of mathematical appendicies which give a concise but full account of the mathematics of the processes involved with star behavior.
Excellent book on this subject
2009/5/2
形式:ハードカバー|Amazonが確認した購入
I was greatly surprised with this book. The author present a detailed view of conservative and non-conservative binary star evolution with many examples, tables and references, exploring different possible scenarios. I use this book often as a reference for my own research. It is excellent for anybody who wants to go deep in the field of binary star evolution. I guess the level is for graduate students, although undergraduates can also find inspiration there.
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