The stability of Galactic open clusters immersed in a gravitating background

Details The stability of Galactic open clusters immersed in a gravitating background The stability of Galactic open clusters immersed in a gravitating background

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6q...8k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, May-June 1990, p. 8-13, 35. In Russian.

Physics

Circular Orbits, Galactic Clusters, Gravitational Fields, Lagrangian Equilibrium Points, Galactic Evolution, Interstellar Magnetic Fields, Quadratures

Scientific paper

Consideration is given to the dynamical evolution of open clusters immersed in a homogeneous gravitating background and rotating along the circular orbit around the center of the Galaxy. Taking into account a tidal approximation of the Galactic field and the commensurability of distances between cluster members, the solution of the generalized Lagrange-Jacobi virial equation leads to quadratures. The results are used to determine the possible types of cluster evolution.

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