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- W162638963 abstract "We calculate some indicators, which are closely related with galaxy clusters' substructure, for each cluster obtained in numerical simulations in OCDM and ΓCDM, and make a statistical comparison between two models. In ΓCDM the indicators, multipole moment power ratios and center shifts, are larger than those in OCDM. This result is consistent with the analytical prediction; galaxy clusters' formation epoch in ΓCDM is later than in OCDM and then clusters in OCDM are more relaxed than those in ΓCDM. We show that these indicators for X-ray surface brightness are useful tools to distinguish between OCDM and ΓCDM." @default.
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- W162638963 date "2003-01-01" @default.
- W162638963 modified "2023-10-14" @default.
- W162638963 title "Substructure of Galaxy Clusters and Cosmological Constant" @default.
- W162638963 cites W3104149101 @default.
- W162638963 doi "https://doi.org/10.1017/s0074180900207699" @default.
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