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- W1505331933 abstract "The papers presented at this symposium show that the theory of a spherical cluster composed of mass points has made great progress: the major processes occurring seem to be well understood in principle. In particular, evaporation and mass stratification account for the early contraction of a cluster core, while the gravothermal instability is responsible for the final collapse. Formation of binaries by three-body encounters can stop the collapse, though the detailed nature of the ensuing expansion is still not fully explored. While further interesting research remains to be done on the evolution of a spherical aggregation of mass points, the broad outlines of the subject seem clear." @default.
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- W1505331933 date "1985-01-01" @default.
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- W1505331933 title "What Next? Priorities in Theory and Observations" @default.
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