Theory of Rotating Stars. (PSA-1), Volume 1 / / Jean-Louis Tassoul.

• Superior document: Title is part of eBook package: De Gruyter Princeton University Press Complete eBook-Package 2014-2015
• VerfasserIn: Tassoul, Jean-Louis,
• Place / Publishing House: Princeton, NJ : : Princeton University Press, , [2015]; ©1979
• Year of Publication: 2015
• Language: English
• Series: Princeton Series in Astrophysics ; 27
• Physical Description: 1 online resource (524 p.)
• Other title: Frontmatter --; Contents --; Preface --; A Short List of Abbreviations --; 1. An Historical Overview --; 2. The Observational Data --; 3. Stellar Hydrodynamics --; 4. Permanent Rotations --; 5. Stellar Models: Techniques --; 6. Small Oscillations and Stability: Techniques --; 7. The Angular Momentum Distribution --; 8. Meridional Circulation --; 9. The Solar Differential Rotation --; 10. Solid-Body Rotation vs. Differential Rotation --; 11. Collapse and Fission --; 12. Stellar Models: Structure and Evolution --; 13. Rotating White Dwarfs --; 14. Oscillations and Stability --; 15. Stellar Magnetism and Rotation --; 16. Rotation in Close Binaries --; Epilogue --; Index of Names --; Index of Subjects
• Format: Mode of access: Internet via World Wide Web.
• ISBN: 9781400868988; 9783110665925; 9783110442496
• DOI: 10.1515/9781400868988
• Access: restricted access
• Hierarchical level: Monograph
• Statement of Responsibility: Jean-Louis Tassoul.

Ever since the first observations of sunspots in the early seventeenth century, stellar rotation has been a major topic in astronomy and astrophysics. Jean-Louis Tassoul synthesizes a large number of theoretical investigations on rotating stars. Drawing upon his own research, Professor Tassoul also carefully critiques various competing ideas. In the first three chapters, the author provides a short historical sketch of stellar rotation, the main observational data on the Sun and other stars on which the subsequent theory is based, and the basic Newtonian hydrodynamics used to study rotating stars. Following a discussion of some general mechanical properties of stars in a state of permanent rotation, he reviews the main techniques for determining the structure of a rotating star and its stability with respect to infinitesimal disturbances. Since the actual distribution of angular momentum within stars is still unknown, Professor Tassoul considers various models of angular momentum as well as of meridional circulation. He devotes the rest of his study to the problems concerning various groups of stars and stages in stellar evolution.Originally published in 1979.The Princeton Legacy Library uses the latest print-on-demand technology to again make available previously out-of-print books from the distinguished backlist of Princeton University Press. These editions preserve the original texts of these important books while presenting them in durable paperback and hardcover editions. The goal of the Princeton Legacy Library is to vastly increase access to the rich scholarly heritage found in the thousands of books published by Princeton University Press since its founding in 1905.