activity
19992009
most citedA unified model for AGN feedback in cosmological simulations of structure formation

890 citations · 6.9k across the 42 of their papers we have counts for

collaborators
Showing 2006 · astro-phShow all

12 papers · 2 filters

astro-ph2006

Cosmic ray feedback in hydrodynamical simulations of galaxy and galaxy cluster formation

Christoph Pfrommer, Volker Springel, Martin Jubelgas +1

It is well known that cosmic rays (CRs) contribute significantly to the pressure of the interstellar medium in our own Galaxy, suggesting that they may play an important role in re…

astro-ph2006140 cited

Simulating cosmic rays in clusters of galaxies - I. Effects on the Sunyaev-Zel'dovich effect and the X-ray emission

Christoph Pfrommer, Torsten A. Ensslin, Volker Springel +2

We performed high-resolution simulations of a sample of 14 galaxy clusters that span a mass range from 5 x 10^13 M_solar/h to 2 x 10^15 M_solar/h to study the effects of cosmic ray…

astro-ph2006125 cited

The first generation of stars in LCDM cosmology

L. Gao, N. Yoshida, T. Abel +3

We have performed a large set of high-resolution cosmological simulations using smoothed particle hydrodynamics to study the formation of the first luminous objects in the LCDM cos…

astro-ph2006304 cited

Formation of z ~ 6 quasars from hierarchical galaxy mergers

Yuexing Li, Lars Hernquist, Brant Robertson +8

The discovery of luminous quasars at redshift z ~ 6 indicates the presence of supermassive black holes (SMBHs) of mass ~10^9 Msun when the Universe was less than one billion years…

astro-ph200684 cited

Physical viscosity in smoothed particle hydrodynamics simulations of galaxy clusters

Debora Sijacki, Volker Springel

Most hydrodynamical simulations of galaxy cluster formation carried out to date have tried to model the cosmic gas as an ideal, inviscid fluid, where only a small amount of (unwant…

astro-ph2006239 cited

Feedback and metal enrichment in cosmological SPH simulations - II. A multiphase model with supernova energy feedback

Cecilia Scannapieco, Patricia B. Tissera, Simon D. M. White +1

We have developed a new scheme to treat a multiphase interstellar medium in smoothed particle hydrodynamics simulations of galaxy formation. This scheme can represent a co-spatial…