activity
20112017
most citedConnecting Angular Momentum and Galactic Dynamics: The complex Interplay between Spin, Mass, and Morphology

266 citations · 1.7k across the 26 of their papers we have counts for

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Showing 2015Show all

9 papers · 1 filter

astro-ph.GA2015

A supernova scenario for magnetic fields and rotation measures in galaxies

Alexander M. Beck, Klaus Dolag

We present a model for the seeding and evolution of magnetic fields in galaxies by supernovae (SN). SN explosions during galaxy assembly provide seed fields, which are subsequently…

astro-ph.CO2015★ 60 cited

nIFTy galaxy cluster simulations II: radiative models

Federico Sembolini, Pascal Jahan Elahi, Frazer R. Pearce +19

We have simulated the formation of a massive galaxy cluster (M = 1.110) in a CDM universe using 10 different codes (RAMSES, 2 in…

astro-ph.GA2015★ 39 cited

nIFTY galaxy cluster simulations III: The Similarity & Diversity of Galaxies & Subhaloes

Pascal J. Elahi, Alexander Knebe, Frazer R. Pearce +17

We examine subhaloes and galaxies residing in a simulated LCDM galaxy cluster () produced by hydrodynamical codes ranging from classic…

astro-ph.IM2015★ 20 cited

Geometrical on-the-fly shock detection in SPH

Alexander M. Beck, K. Dolag, Julius M. F. Donnert

We present an on-the-fly geometrical approach for shock detection and Mach number calculation in simulations employing smoothed particle hydrodynamics (SPH). We utilize pressure gr…

astro-ph.CO2015★ 211 cited

Cool Core Clusters from Cosmological Simulations

E. Rasia, S. Borgani, G. Murante +7

We present results obtained from a set of cosmological hydrodynamic simulations of galaxy clusters, aimed at comparing predictions with observational data on the diversity between…

astro-ph.CO2015★ 46 cited

Neutral hydrogen in galaxy clusters: impact of AGN feedback and implications for intensity mapping

Francisco Villaescusa-Navarro, Susana Planelles, Stefano Borgani +8

By means of zoom-in hydrodynamic simulations we quantify the amount of neutral hydrogen (HI) hosted by groups and clusters of galaxies. Our simulations, which are based on an impro…