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• W3103454771 abstract "The discrepancy between mass estimates from X-ray and strong gravitational lensing analyses has recently been pointed out for several clusters, in particular A1689 and A2218. We analyze the internal structures of these clusters by applying a recent development of the method of wavelet analysis, which uses the complete information obtained from optical data, i.e., galaxy positions and redshifts. We find that both clusters show the presence of structures superimposed along the line of sight with different mean redshifts and smaller velocity dispersions than the system as a whole, suggesting that the clusters could be cases of the ongoing merging of clumps." @default.
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• W3103454771 date "1997-11-20" @default.
• W3103454771 modified "2023-10-17" @default.
• W3103454771 title "New Optical Insights into the Mass Discrepancy of Galaxy Clusters: The Cases of A1689 and A2218" @default.
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• W3103454771 doi "https://doi.org/10.1086/304866" @default.
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