MARC Record from Library of Congress

LEADER: 02815nam a22002778a 4500
001 2009034267
003 DLC
005 20090828113001.0
008 090818s2009 nyu 000 0 eng
010 $a 2009034267
020 $a9780521866040 (hardback)
040 $aDLC$cDLC
050 00 $aQB808$b.P75 2009
082 00 $a523.8/8$222
100 1 $aPrialnik, Dina.
245 13 $aAn introduction to the theory of stellar structure and evolution /$cDina Prialnik.
250 $a2nd ed.
260 $aNew York :$bCambridge University Press,$c2009.
263 $a0911
300 $ap. cm.
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.
505 8 $aMachine generated contents note: 1. Observations and assumptions; 2. Equations of stellar evolution; 3. Physics of gas and radiation; 4. Nuclear processes; 5. Equilibrium - simple models; 6. Stability of stars; 7. Evolution of stars - schematic picture; 8. Mass loss from stars; 9. The evolution of stars - a detailed picture; 10. Exotic stars: supernovae, pulsars, black holes; 11. Interacting binary stars; 12. The stellar life cycle; Appendixes; References; Index.
650 0 $aStars$xStructure.
650 0 $aStars$xEvolution.
856 42 $3Cover image$uhttp://assets.cambridge.org/97805218/66040/cover/9780521866040.jpg