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Part I. Basic Phenomenology: 1. Scales; 2. Observational windows; 3. Classifications; 4. Photometry, kinematics, dark matter; 5. Basic questions, semi-empirical approach, dynamical window; Part II. Physical Models: 6. Self-gravity and relation with plasma physics; 7. Relaxation times, absence of thermodynamical equilibrium; 8. Models; 9. Equilibrium and stability: symmetry and symmetry breaking; 10. Classical ellipsoids; 11. Introduction to dispersive waves; 12. Jeans instability; Part III. Spiral Galaxies: 13. Orbits; 14. The basic state: vertical and horizontal equilibrium in the disk; 15. Density waves; 16. Role of gas; 17. Global spiral modes; 18. Spiral structure in galaxies; 19. Bending waves; 20. Dark matter in spiral galaxies; Part IV. Elliptical Galaxies: 21. Orbits; 22. Stellar dynamical approach; 23. Stability; 24. Dark matter in elliptical galaxies; Part V. In Perspective: 25. Selected aspects of formation and evolution; Notes; Index.
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Add Dynamics of Galaxies, Our understanding of galaxies has advanced significantly in recent years. Powerful computer simulations and detailed observations from ground- and space-based telescopes have been instrumental in this. This graduate textbook provides students with a compl, Dynamics of Galaxies to the inventory that you are selling on WonderClubX
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Add Dynamics of Galaxies, Our understanding of galaxies has advanced significantly in recent years. Powerful computer simulations and detailed observations from ground- and space-based telescopes have been instrumental in this. This graduate textbook provides students with a compl, Dynamics of Galaxies to your collection on WonderClub |