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.
2000
Large Scale Structure in the X-ray Universe
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/1361662
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