The Structure, Stability, and Dynamics
of Self-Gravitating Systems

Joel E. Tohline
tohline@rouge.phys.lsu.edu

REFERENCES

  1. Arfken, George. 1985, Mathematical Methods for Physicists, (New York: Academic Press: QAQA37.2.A74: ISBN 0-12-059820-5).

  2. Binney, J. and Tremaine, S. 1987, Galactic Dynamics, (Princeton, NJ: Princeton Univ. Press).

  3. Chandrasekhar, S. 1967, An Introduction to the Study of Stellar Structure, (New York: Dover: QB801.C479: ISBN 0-486-60413-6).

  4. Chandrasekhar, S. 1987, Ellipsoidal Figures of Equilibrium, (New York: Dover: QB410.C47: ISBN 0-486-65258-0).

  5. Hayashi, C., Narita, S., and Miyama, S.M. 1982, Analytic Solutions for Equilibrium of Rotating Isothermal Clouds, Progress of Theoretical Physics, Volume 68, No. 6, pp. 1949-1966.

  6. Landau, L.D. and Lifshitz, E. M. 1975, Fluid Mechanics, (New York: Pergamon Press).

  7. MacLaurin, Colin. 1742. A Treatise on Fluxions.

  8. Tassoul, Jean-Louis 1978, Theory of Rotating Stars, (Princeton, NJ: Princeton Univ. Press).

Home Page | Preface | Context | Applications | Appendices | Search Index