真繁荣
发表于 2025-3-27 01:00:05
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forthy
发表于 2025-3-27 02:21:30
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树胶
发表于 2025-3-27 08:58:03
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男生如果明白
发表于 2025-3-27 11:29:33
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opalescence
发表于 2025-3-27 17:16:15
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OVER
发表于 2025-3-27 17:53:29
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convert
发表于 2025-3-27 23:33:14
Women in the English Novel, 1800-1900open clusters whereas the “halo” red clusters are less massive and younger than the galactic globulars (Kontizas, Danezis, Kontizas, 1982; Kontizas and Kontizas, 1983). (b) All clusters show density profiles that fit the available theoretical models (King, 1962) giving evidence of relaxed systems, e
ineptitude
发表于 2025-3-28 05:58:31
https://doi.org/10.1007/978-1-349-08184-4part of a major study of globular cluster core structure. These data are being used to test for the presence of central cusps in the surface brightness profiles; which are expected to be present in clusters which have already undergone core collapse (Cohn and Hut 1984).
terazosin
发表于 2025-3-28 09:54:46
Von der Schule in die Arbeitsweltrom the centre to the edge and the ordered to random motions ratios are deduced for two globular clusters: ω Cen and 47 Tuc. Masses through virial theorem and M/L ratios are also given. A more comprehensive study will be published in Astron. & Astrophys.
Lipohypertrophy
发表于 2025-3-28 13:48:27
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