Artigo Revisado por pares

Dynamics of Globular Clusters

1984; American Association for the Advancement of Science; Volume: 225; Issue: 4661 Linguagem: Inglês

10.1126/science.225.4661.465

ISSN

1095-9203

Autores

Lyman Spitzer,

Tópico(s)

High-pressure geophysics and materials

Resumo

In their attempt to reach kinetic equilibrium, through gravitational encounters between separate stars, globular clusters are driven to destruction, with their cores collapsing and their outer regions expanding. The effects of core collapse, which apparently produces x-ray sources, are not yet fully understood, but white dwarfs and neutron stars, probably in binary systems, are thought to be involved, and possibly black holes as well.

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