chandel 发表于 2025-3-23 12:28:11
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Precollapse Evolution of Globular Clusterso modify the system so that it approaches a more probable configuration. In statistical equilibrium, the distribution of stars among states of different energy, E., per unit mass would be determined to a first approximation by the probability P., where . here g. is the statistical weight of each sta巧办法 发表于 2025-3-24 01:20:06
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https://doi.org/10.1007/978-1-349-07805-9Proper motion data of Ml3 cluster members are very useful for the investigation of the cluster’s internal dynamics. We introduce a maximum likelihood method to fit these data in terms of conventional King-Michie models.闪光东本 发表于 2025-3-24 15:03:42
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