A globular-cluster model with variable mean mass of a single star.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Globular Clusters: Models

Scientific paper

The application of the basic hydrodynamical equations to globular clusters is reconsidered. As usually, these stellar systems are assumed to be spherically symmetric and in a steady state with an isotropic velocity distribution. A system of differential equations with four independent functions describing a globular-cluster model is developed. The obtained results show that it is possible to find a solution with two input empirical functions describing the spatial distribution of stars and the variation of the mean mass of a single star.

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