Abstract
A new numerical method is proposed for solving the problems connected with the evolution of spherical clusters. The method is based upon the solution of the algebraic equations describing the motions of spherical shells.
The stage of the collapse of a typical cluster is considered. The initial configuration is taken as a system with a uniform density distribution and with velocities much less than the virial ones. The model close to a stationary one has been obtained. The mass of the stationary cluster comprises about 60% of the initial one. The density distribution of the outer part of the cluster approximately corresponds to a profile of ρ ∝R −3.3.
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References
Dekel, A., Kowitt, M., and Shaham, J.: 1981, Preprint OAP-613.
Gott, J. R.: 1975,Astrophys. J. 201, 296.
Gott, J. R.: 1977,Ann. Rev. Astron. Astrophys. 15, 235.
Hénon, M.: 1964,Ann. Astrophys. 27, 83.
Hogan, C.: 1979,Monthly Notices Roy. Astron. Soc. 188, 781.
Landau, L. D. and Lifshitz, E. M.: 1965,Mechanika, M., Nauka.
Lynden-Bell, D.: 1967,Monthly Notices Roy. Astron. Soc. 136, 101.
Peebles, P. J. E.: 1970,Astrophys. J. 75, 13.
Spitzer, J. L. and Hart, H. M.: 1971,Astrophys. J. 164, 399.
Spitzer, J. L. and Shapiro, L. S.: 1972,Astrophys. J. 173, 529.
Yangurazova, L. R.: 1981, ‘Evolutcionnaya model sfericheski symmetrichnoy systemi tochechnih chastic, vzaimodeystvuuysih obratno proporicionalno kvadratu rasstoyaniya mezdi nimi. Algorithmi i programmi’,Inf. Bull. Gos FAP, No. 5 (43).
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Yangurazova, L.R., Bisnovatyi-Kogan, G.S. Collapse of the spherical stellar system. Astrophys Space Sci 100, 319–328 (1984). https://doi.org/10.1007/BF00651607
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DOI: https://doi.org/10.1007/BF00651607