Schlemms-Canal
发表于 2025-4-1 04:53:14
The Disruption Time of Clusters in Selected Regions of Four Galaxies,od. The values of . are the same within their uncertainties in the four galaxies with .. However, the disruption time .. of clusters of . is very different in the different locations. It is shortest in the inner region of M51 ( .. = 4 x 10. yrs) and highest in the SMC ( .. = 4 x 10. yrs).
flex336
发表于 2025-4-1 07:58:13
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brassy
发表于 2025-4-1 12:29:25
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我正派
发表于 2025-4-1 14:24:42
Young Massive Clusters in Normal Galaxies,ampling from a power-law luminosity function, suggesting that statistical effects can account for some of the apparent differences between cluster populations in various environments. It is still unclear to what extent the underlying . distribution of young stellar clusters might be affected by physical properties of the parent galaxies.
男生戴手铐
发表于 2025-4-1 18:58:58
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machination
发表于 2025-4-1 23:34:30
Globular Cluster Formation,cluster formation. Empirically it appears that globular cluster formation occurs preferentially in regions in which star formation occurs at a high rate and efficiency. Further, the interstellar medium in such regions is likely to be at a higher pressure than less active star-forming environments. A
里程碑
发表于 2025-4-2 04:04:52
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HAVOC
发表于 2025-4-2 08:12:35
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