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• 001 0000605591

• 003 CAL

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• 006 m_ d

• 007 cr cn

• 008 090818s2010 enka sb 001 0 eng

• 010 __ |a 2009034267

• 020 __ |a 9781316283165

• 020 __ |a 9780521866040

• 040 __ |a DLC |c DLC |d BTCTA |d YDXCP |d C#P |d CDX |d UKM |d DLC

• 050 00 |a QB808 |b .P75 2010

• 082 00 |a 523.8/8 |2 22

• 093 __ |a P15 |2 4

• 100 1_ |a Prialnik, Dina.

• 245 13 |a An introduction to the theory of stellar structure and evolution |h [electronicresource] / |c Dina Prialnik.

• 250 __ |a 2nd ed.

• 260 __ |a Cambridge ; |a New York : |b Cambridge University Press, |c c2010.

• 300 __ |a 1 online resource (xv, 314 p.) : |b ill.

• 500 __ |a Descriptionbasedonprintversionrecord.

• 504 __ |a Includes bibliographical references and index.

• 505 0_ |a Observational background and basic assumptions -- The equations of stellar evolution -- Elementary physics of gas and radiation in stellar interiors -- Nuclear processes that take place in stars -- Equilibrium stellar configurations--simple models -- The stability of stars -- The evolution of stars--a schematic picture -- Mass loss from stars -- The evolution of stars--a detailed picture -- Exotic stars : supernovae, pulsars and black holes -- Interacting binary stars -- The stellar life cycle.

• 520 __ |a "Using fundamental physics, the theory of stellar structure and evolution can predict how stars are born, how their complex internal structure changes, what nuclear fuel they burn, and their ultimate fate. This textbook is a stimulating introduction for undergraduates in astronomy, physics and applied mathematics, taking a course on the physics of stars. It uniquely emphasizes the basic physical principles governing stellar structure and evolution. This second edition contains two new chapters on mass loss from stars and interacting binary stars, and new exercises. Clear and methodical, it explains the processes in simple terms, while maintaining mathematical rigor. Starting from general principles, this textbook leads students step-by-step to a global, comprehensive understanding of the subject. Fifty exercises and full solutions allow students to test their understanding. No prior knowledge of astronomy is required, and only a basic background in physics and mathematics is necessary"--Provided by publisher.

• 520 __ |a "Stellar evolution calculations have made great progress in recent years, following the rapid development of computational means: increasingly faster CPUs and greater memory volumes. Nevertheless, I have made use of new results only when they provide better illustration for points raised in text. For themost part, old results are still valid and this long-term validity is worth emphasizing; the theory of stellar structure and evolution, with all its complexity, is a well-established physical theory. The text was"--Provided by publisher.

• 650 _0 |a Stars |x Structure.

• 650 _0 |a Stars |x Evolution.

• 856 4_ |u http://www.itextbook.cn/f/book/bookDetail?bookId=9954b4c5b4f645c1a5fe5ee33e1150f5 |z An electronic book accessible through the World Wide Web; click to view