High-resolution cosmological hydrodynamical simulations are used for studying the evolution and the properties of the gas contained in the filamentary structure connecting galaxy clusetrs.
Formation and Evolution of X--ray Filaments between Galaxy Clusters
PANTANO, ORNELLA;
2000
Abstract
High-resolution cosmological hydrodynamical simulations are used for studying the evolution and the properties of the gas contained in the filamentary structure connecting galaxy clusetrs.File in questo prodotto:
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