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19932026
most citedSubstructures in hydrodynamical cluster simulations

1.1k citations · 25k across the 321 of their papers we have counts for

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Showing 2018Show all

10 papers · 1 filter

astro-ph.GA2018★ 22 cited

The seeds of supermassive black holes and the role of local radiation and metal spreading

U. Maio, S. Borgani, B. Ciardi +1

We present cosmological hydrodynamical simulations including atomic and molecular non-equilibrium chemistry, multi-frequency radiative transfer (0.7-100 eV sampled over 150 frequen…

astro-ph.CO2018★ 12 cited

nIFTy Galaxy Cluster simulations VI: The dynamical imprint of substructure on gaseous cluster outskirts

C. Power, P. J. Elahi, C. Welker +11

Galaxy cluster outskirts mark the transition region from the mildly non-linear cosmic web to the highly non-linear, virialised, cluster interior. It is in this transition region th…

astro-ph.CO2018★ 39 cited

Athena X-IFU synthetic observations of galaxy clusters to probe the chemical enrichment of the Universe

E. Cucchetti, E. Pointecouteau, P. Peille +14

Answers to the metal production of the Universe can be found in galaxy clusters, notably within their Intra-Cluster Medium (ICM). The X-ray Integral Field Unit (X-IFU) on board the…

astro-ph.GA2018★ 231 cited

The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications

Weiguang Cui, Alexander Knebe, Gustavo Yepes +34

We introduce the THE THREE HUNDRED project, an endeavour to model 324 large galaxy clusters with full-physics hydrodynamical re-simulations. Here we present the data set and study…

astro-ph.GA2018★ 302 cited

Observations of the MIssing Baryons in the warm-hot intergalactic medium

F. Nicastro, J. Kaastra, Y. Krongold +18

It has been known for decades that the observed number of baryons in the local universe falls about 30-40% short of the total number of baryons predicted by Big-Bang Nucleosynthesi…

astro-ph.GA2018★ 10 cited

Colour-magnitude diagram in simulations of galaxy formation

Milena Valentini, Alessandro Bressan, Stefano Borgani +3

State-of-the-art cosmological hydrodynamical simulations have star particles with typical mass between and M according to resolution, and treat th…