activity
20102026
most citedThe Romulus Cosmological Simulations: A Physical Approach to the Formation, Dynamics and Accretion Models of SMBHs

335 citations · 3.5k across the 72 of their papers we have counts for

collaborators
Showing 2021Show all

9 papers · 1 filter

astro-ph.GA2021★ 33 cited

Massive Black Hole Mergers with Orbital Information: Predictions from the ASTRID Simulation

Nianyi Chen, Yueying Ni, A. Miguel Holgado +6

We examine massive black hole (MBH) mergers and their associated gravitational wave signals from the large-volume cosmological simulation Astrid. Astrid includes galaxy formation a…

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★ 144 cited

The ASTRID simulation: the evolution of Supermassive Black Holes

Yueying Ni, Tiziana Di Matteo, Simeon Bird +6

We present the evolution of black holes (BHs) and their relationship with their host galaxies in Astrid, a large-volume cosmological hydrodynamical simulation with box size 250 $h^…

astro-ph.GA2021★ 31 cited

What's in a name? Quantifying the interplay between the Definition, Orientation, and Shape of Ultra-diffuse Galaxies Using the Romulus Simulations

Jordan D. Van Nest, F. Munshi, A. C. Wright +4

We explore populations of ultra-diffuse galaxies (UDGs) in isolated, satellite, and cluster environments using the Romulus25 and RomulusC simulations, including how the populations…

astro-ph.GA2021★ 42 cited

Unveiling the Population of Wandering Black Holes via Electromagnetic Signatures

Angelo Ricarte, Michael Tremmel, Priyamvada Natarajan +1

While most galaxies appear to host a central supermassive black hole (SMBH), they are expected to also contain a substantial population of off-center "wandering" SMBHs naturally pr…

astro-ph.GA2021★ 24 cited

The Impact of Cosmic Rays on the Kinematics of the Circumgalactic Medium

Iryna S. Butsky, Jessica K. Werk, Kirill Tchernyshyov +9

We use hydrodynamical simulations of two Milky Way-mass galaxies to demonstrate the impact of cosmic-ray pressure on the kinematics of cool and warm circumgalactic gas. Consistent…

astro-ph.GA2021★ 76 cited

Dynamical Friction Modeling of Massive Black Holes in Cosmological Simulations and Effects on Merger Rate Predictions

Nianyi Chen, Yueying Ni, Michael Tremmel +4

In this work we establish and test methods for implementing dynamical friction for massive black hole pairs that form in large volume cosmological hydrodynamical simulations which…

astro-ph.GA2021★ 80 cited

Origins and Demographics of Wandering Black Holes

Angelo Ricarte, Michael Tremmel, Priyamvada Natarajan +2

We characterise the population of wandering black holes, defined as those physically offset from their halo centres, in the Romulus cosmological simulations. Unlike most other curr…

astro-ph.GA2021★ 62 cited

The Origins of Off-Centre Massive Black Holes in Dwarf Galaxies

Jillian M. Bellovary, Sarra Hayoune, Katheryn Chafla +9

Massive black holes often exist within dwarf galaxies, and both simulations and observations have shown that a substantial fraction of these may be off-center with respect to their…