activity
20032026
most citedDancing in the dark: galactic properties trace spin swings along the cosmic web

888 citations · 7.3k across the 106 of their papers we have counts for

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Showing 2016Show all

5 papers · 1 filter

astro-ph.CO2016★ 25 cited

Projected Axis Ratios of Galaxy Clusters in the Horizon-AGN Simulation: Impact of Baryon Physics and Comparison with Observations

Daichi Suto, Sebastien Peirani, Yohan Dubois +4

We characterize the non-sphericity of galaxy clusters by the projected axis ratio of spatial distribution of star, dark matter, and X-ray surface brightness (XSB). We select 40 sim…

astro-ph.GA2016★ 145 cited

Density profile of dark matter haloes and galaxies in the Horizon-AGN simulation: the impact of AGN feedback

S. Peirani, Y. Dubois, M. Volonteri +7

Using a suite of three large cosmological hydrodynamical simulations, Horizon-AGN, Horizon-noAGN (no AGN feedback) and Horizon-DM (no baryons), we investigate how a typical sub-gri…

astro-ph.GA2016★ 495 cited

The Horizon-AGN simulation: morphological diversity of galaxies promoted by AGN feedback

Yohan Dubois, Sebastien Peirani, Christophe Pichon +4

The interplay between cosmic gas accretion on to galaxies and galaxy mergers drives the observed morphological diversity of galaxies. By comparing the state-of-the-art hydrodynamic…

astro-ph.GA2016★ 198 cited

Suppressing star formation in quiescent galaxies with supermassive black hole winds

Edmond Cheung, Kevin Bundy, Michele Cappellari +22

Quiescent galaxies with little or no ongoing star formation dominate the galaxy population above , where their numbers have increased by a fac…

astro-ph.GA2016★ 149 cited

On the number density of "direct collapse" black hole seeds

Melanie Habouzit, Marta Volonteri, Muhammad Latif +2

Supermassive black holes (BHs) of millions solar masses and above reside in the center of most local galaxies, but they also power active galactic nuclei and quasars, detected up t…