Search Results - "G, Murante"
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Substructures in hydrodynamical cluster simulations
Published in Monthly notices of the Royal Astronomical Society (21-10-2009)“…The abundance and structure of dark matter subhaloes have been analysed extensively in recent studies of dark-matter-only simulations, but comparatively little…”
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The relation between velocity dispersion and mass in simulated clusters of galaxies: dependence on the tracer and the baryonic physics
Published in Monthly notices of the Royal Astronomical Society (21-04-2013)“…We present an analysis of the relation between the masses of cluster- and group-sized haloes, extracted from Λ cold dark matter (ΛCDM) cosmological N-body and…”
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ON THE NATURE OF HYDROSTATIC EQUILIBRIUM IN GALAXY CLUSTERS
Published in The Astrophysical journal (20-08-2016)“…ABSTRACT In this paper, we investigate the level of hydrostatic equilibrium (HE) in the intracluster medium of simulated galaxy clusters, extracted from…”
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BCG Mass Evolution in Cosmological Hydro-Simulations
Published in Monthly notices of the Royal Astronomical Society (01-09-2018)Get full text
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The origin of ICM enrichment in the outskirts of present-day galaxy clusters from cosmological hydrodynamical simulations
Published in Monthly notices of the Royal Astronomical Society (11-05-2018)“…Abstract The uniformity of the intracluster medium (ICM) enrichment level in the outskirts of nearby galaxy clusters suggests that chemical elements were…”
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On the role of AGN feedback on the thermal and chemodynamical properties of the hot intracluster medium
Published in Monthly notices of the Royal Astronomical Society (11-02-2014)“…We present an analysis of the properties of the intracluster medium (ICM) in an extended set of cosmological hydrodynamical simulations of galaxy clusters and…”
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Simulating the effect of active galactic nuclei feedback on the metal enrichment of galaxy clusters
Published in Monthly notices of the Royal Astronomical Society (21-01-2010)“…We present a study of the effect of active galactic nuclei (AGN) feedback on metal enrichment and thermal properties of the intracluster medium (ICM) in…”
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Baryon census in hydrodynamical simulations of galaxy clusters
Published in Monthly notices of the Royal Astronomical Society (11-05-2013)“…We carry out an analysis of a set of cosmological smoothed particle hydrodynamics (SPH) hydrodynamical simulations of galaxy clusters and groups aimed at…”
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The Aquila comparison project: the effects of feedback and numerical methods on simulations of galaxy formation
Published in Monthly notices of the Royal Astronomical Society (01-06-2012)“…We compare the results of various cosmological gas-dynamical codes used to simulate the formation of a galaxy in the Λ cold dark matter structure formation…”
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Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution
Published in Monthly notices of the Royal Astronomical Society (01-03-2018)“…AbstractWe analyse cosmological hydrodynamical simulations of galaxy clusters to study the X-ray scaling relations between total masses and observable…”
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Pressure of the hot gas in simulations of galaxy clusters
Published in Monthly notices of the Royal Astronomical Society (01-06-2017)“…Abstract We analyse the radial pressure profiles, the intracluster medium (ICM) clumping factor and the Sunyaev–Zel'dovich (SZ) scaling relations of a sample…”
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An improved SPH scheme for cosmological simulations
Published in Monthly notices of the Royal Astronomical Society (11-01-2016)“…We present an implementation of smoothed particle hydrodynamics (SPH) with improved accuracy for simulations of galaxies and the large-scale structure. In…”
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The history of chemical enrichment in the intracluster medium from cosmological simulations
Published in Monthly notices of the Royal Astronomical Society (11-06-2017)“…Abstract The distribution of metals in the intracluster medium (ICM) of galaxy clusters provides valuable information on their formation and evolution, on the…”
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Dynamical difference between the cD galaxy and the diffuse, stellar component in simulated galaxy clusters
Published in Monthly notices of the Royal Astronomical Society (01-07-2010)“…Member galaxies within galaxy clusters nowadays can be routinely identified in cosmological, hydrodynamical simulations using methods based on identifying self…”
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Characterizing diffused stellar light in simulated galaxy clusters
Published in Monthly notices of the Royal Astronomical Society (01-01-2014)“…In this paper, we carry out a detailed analysis of the performance of two different methods to identify the diffuse stellar light in cosmological…”
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A non-ideal magnetohydrodynamic gadget: simulating massive galaxy clusters
Published in Monthly notices of the Royal Astronomical Society (01-12-2011)“…Magnetic fields in the intra-cluster medium (ICM) of galaxy clusters have been studied in the past through different methods. So far, our understanding of the…”
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X-ray mass proxies from hydrodynamic simulations of galaxy clusters - I
Published in Monthly notices of the Royal Astronomical Society (01-09-2011)“…Using extended sets of cosmological hydrodynamical simulations of galaxy clusters, we present a detailed study of scaling relations between total cluster mass…”
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Machine learning to identify ICL and BCG in simulated galaxy clusters
Published in Monthly notices of the Royal Astronomical Society (22-06-2022)“…ABSTRACT Nowadays, Machine Learning techniques offer fast and efficient solutions for classification problems that would require intensive computational…”
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Simulating the evolution of disc galaxies in a group environment – II. The influence of close encounters between galaxies
Published in Monthly notices of the Royal Astronomical Society (11-10-2014)“…We study the evolution of disc galaxies in group environments under the effect of both the global tidal field and close encounters between galaxies, using…”
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Evolution and role of mergers in the BCG–cluster alignment. A view from cosmological hydrosimulations
Published in Monthly notices of the Royal Astronomical Society (21-06-2020)“…ABSTRACT Contradictory results have been reported on the time evolution of the alignment between clusters and their brightest cluster galaxy (BCG). We study…”
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