Fluid Techniques and Evolution of Anisotropy
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[1] Tse-Hao Ko. The influence of pyrolysis on physical properties and microstructure of modified PAN fibers during carbonization , 1991 .
[2] D. Heggie,et al. Statistics of N-body simulations – I. Equal masses before core collapse , 1993, astro-ph/9305008.
[3] J. Breeden,et al. The onset of gravothermal oscillations in globular cluster evolution , 1994 .
[4] R. Spurzem. Evolution of Stars and Gas in Galactic Nuclei , 1992 .
[5] R. Spurzem. Gravothermal instability of anisotropic self-gravitating gas spheres : singular equilibrium solution , 1991 .
[6] P. P. Eggleton,et al. On the consequences of the gravothermal catastrophe , 1980 .
[7] Astronomer Royal,et al. The gravo-thermal catastrophe in isothermal spheres and the onset of red-giant structure for stellar systems , 1968 .
[8] K. Nomoto,et al. Gravothermal Catastrophe of Finite Amplitude , 1978 .
[9] R. Larson. A Model for the Formation of a Spherical Galaxy , 1969 .
[10] James E. Gunn,et al. Dynamical Studies of Globular Clusters Based on Photoelectric Radial Velocities of Individual Stars and on the Observed Mass Function. II. M13 , 1987 .
[11] P. Hut,et al. Gravothermal oscillations after core collapse in globular cluster evolution , 1989 .
[12] S. Inagaki,et al. A gas model for multicomponent star clusters: method and comparison with Fokker-Planck theory , 1985 .
[13] Piet Hut,et al. Binary-single-star scattering. V: Steady state binary distribution in a homogeneous static background of single stars , 1993 .
[14] Rainer Spurzem,et al. Anisotropic gaseous models for the evolution of star clusters , 1991 .
[15] R. Larson. A Method for Computing the Evolution of Star Clusters , 1970 .
[16] H. Cohn,et al. Numerical integration of the Fokker-Planck equation and the evolution of star clusters , 1979 .
[17] H. Cohn. Direct Fokker-Planck calculations. , 1985 .
[18] R. Larson. The Evolution of Star Clusters , 1970 .
[19] Daiichiro Sugimoto,et al. Gravothermal Catastrophe and Negative Specific Heat of Self-Gravitating Systems , 1978 .
[20] D. Sugimoto,et al. Post-collapse evolution and gravothermal oscillation of globular clusters , 1984 .
[21] H. Cohn,et al. Late core collapse in star clusters and the gravothermal instability , 1980 .
[22] D. Heggie. Post-collapse evolution of a gaseous cluster model , 1984 .
[23] P. Hut. Binary Formation and Interactions with Field Stars , 1985 .