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- W2017622219 abstract "High-resolution N-body simulations are used to investigate systematic trends in the mass profiles and total masses of clusters as derived from three simple estimators: (1) the weak gravitational lensing shear field, under the assumption of an isothermal cluster potential; (2) the dynamical mass obtained from the measured velocity dispersion, under the assumption of an isothermal cluster potential; and (3) the classical virial estimator. The clusters used for the analysis were obtained from simulations of a standard cold dark matter universe at z = 0.5 and consist of order × 105 particles of mass mp ≃ 1010 M☉. The clusters are not smooth and spherically symmetric but, rather, the mass distribution is triaxial, and significant substructure exists within the clusters. Not surprisingly, the level of agreement between the cluster mass profiles obtained from the various estimators and the actual mass profiles is found to be scale-dependent." @default.
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- W2017622219 date "1999-10-10" @default.
- W2017622219 modified "2023-09-30" @default.
- W2017622219 title "A Comparison of Simple Mass Estimators for Galaxy Clusters" @default.
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- W2017622219 doi "https://doi.org/10.1086/307793" @default.
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