Titlebook: Extragalactic Globular Cluster Systems; Proceedings of the E Markus Kissler-Patig Conference proceedings 2003 Springer-Verlag Berlin Heidel

Schlemms-Canal

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

brassy

我正派

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.

男生戴手銬

machination

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

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HAVOC