Orbital stability of spherical galactic models

Author:

Lemou Mohammed,Méhats Florian,Raphaël Pierre

Publisher

Springer Science and Business Media LLC

Subject

General Mathematics

Reference49 articles.

1. Aly, J.-J.: On the lowest energy state of a collisionless self-gravitating system under phase volume constraints. Mon. Not. R. Astron. Soc. 241, 15 (1989)

2. Antonov, A.V.: Remarks on the problem of stability in stellar dynamics. Sov. Astron. 4, 859–867 (1961)

3. Antonov, A.V.: Solution of the problem of stability of a stellar system with the Emden density law and spherical velocity distribution. J. Leningr. Univ. Ser. Mekh. Astron. 7, 135–146 (1962)

4. Arsen’ev, A.A.: Global existence of a weak solution of Vlasov’s system of equations. U.S.S.R. Comput. Math. Math. Phys. 15, 131–141 (1975)

5. Batt, J., Faltenbacher, W., Horst, E.: Stationary spherically symmetric models in stellar dynamics. Arch. Ration. Mech. Anal. 93, 159–183 (1986)

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