activity
20072026
most citedDancing in the dark: galactic properties trace spin swings along the cosmic web

888 citations · 13.4k across the 233 of their papers we have counts for

collaborators
Showing 2021Show all

10 papers · 1 filter

astro-ph.GA2021

Dual AGN in the Horizon-AGN simulation and their link to galaxy and massive black hole mergers, with an excursus on multiple AGN

Marta Volonteri, Hugo Pfister, Ricarda Beckmann +5

The occurrence of dual active galactic nuclei (AGN) on scales of a few tens of kpc can be used to study merger-induced accretion on massive black holes (MBHs) and to derive clues o…

astro-ph.GA2021★ 72 cited

Supermassive black holes in cosmological simulations II: the AGN population and predictions for upcoming X-ray missions

Melanie Habouzit, Rachel S. Somerville, Yuan Li +13

In large-scale hydrodynamical cosmological simulations, the fate of massive galaxies is mainly dictated by the modeling of feedback from active galactic nuclei (AGN). The amount of…

astro-ph.GA2021

Momentum deposition of supernovae with cosmic rays

Francisco Rodríguez Montero, Sergio Martin-Alvarez, Debora Sijacki +3

The cataclysmic explosions of massive stars as supernovae are one of the key ingredients of galaxy formation. However, their evolution is not well understood in the presence of mag…

astro-ph.GA2021

Gravitational torques dominate the dynamics of accreted gas at

Corentin Cadiou, Yohan Dubois, Christophe Pichon

Galaxies form from the accretion of cosmological infall of gas. In the high redshift Universe, most of this gas infall is expected to be dominated by cold filamentary flows which c…

astro-ph.GA2021★ 1 cited

The NewHorizon Simulation -- To Bar Or Not To Bar

J. Reddish, K. Kraljic, M. S. Petersen +12

We use the NewHorizon simulation to study the redshift evolution of bar properties and fractions within galaxies in the stellar masses range $M_{\star} = 10^{7.25} - 10^{11.4} \ \r…

astro-ph.CO2021★ 22 cited

I- A hydrodynamical CLONE of the Virgo cluster of galaxies to confirm observationally-driven formation scenarios

Jenny G. Sorce, Yohan Dubois, Jeremy Blaizot +3

At ~16-17Mpc from us, the Virgo cluster is a formidable source of information to study cluster formation and galaxy evolution in rich environments. Several observationally-driven f…