activity
20072017
most citedForming Realistic Late-Type Spirals in a LCDM Universe: The Eris Simulation

527 citations · 2k across the 17 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

8 papers · 1 filter

astro-ph.CO2012★ 78 cited

Massive black hole seeds born via direct gas collapse in galaxy mergers: their properties, statistics and environment

Silvia Bonoli, Lucio Mayer, Simone Callegari

We study the statistics and cosmic evolution of massive black hole seeds formed during major mergers of gas-rich late-type galaxies. Generalizing the results of the hydro-simulatio…

astro-ph.CO2012★ 69 cited

Formation and Hardening of Supermassive Black Hole Binaries in Minor Mergers of Disk Galaxies

Fazeel Mahmood Khan, Ingo Berentzen, Peter Berczik +4

We model for the first time the complete orbital evolution of a pair of Supermassive Black Holes (SMBHs) in a 1:10 galaxy merger of two disk dominated gas-rich galaxies, from the s…

astro-ph.CO2011★ 179 cited

Observability of Dual Active Galactic Nuclei in Merging Galaxies

Sandor Van Wassenhove, Marta Volonteri, Lucio Mayer +3

Supermassive black holes (SMBHs) have been detected in the centers of most nearby massive galaxies. Galaxies today are the products of billions of years of galaxy mergers, but also…

astro-ph.CO2011★ 527 cited

Forming Realistic Late-Type Spirals in a LCDM Universe: The Eris Simulation

Javiera Guedes, Simone Callegari, Piero Madau +1

Simulations of the formation of late-type spiral galaxies in a cold dark matter LCDM universe have traditionally failed to yield realistic candidates. Here we report a new cosmolog…

astro-ph.CO2010★ 7 cited

Tidal stirring of Milky Way satellites: a simple picture with the integrated tidal force

Ewa L. Lokas, Stelios Kazantzidis, Lucio Mayer +1

Most of dwarf spheroidal galaxies in the Local Group were probably formed via environmental processes like the tidal interaction with the Milky Way. We study this process via N-bod…

astro-ph.CO2010★ 155 cited

On the Efficiency of the Tidal Stirring Mechanism for the Origin of Dwarf Spheroidals: Dependence on the Orbital and Structural Parameters of the Progenitor Disky Dwarfs

Stelios Kazantzidis, Ewa L. Lokas, Simone Callegari +2

(Abridged) The tidal stirring model posits the formation of dSph galaxies via the tidal interactions between rotationally-supported dwarfs and MW-sized host galaxies. Using a set o…

astro-ph.CO2010★ 118 cited

Growing Massive Black Hole Pairs in Minor Mergers of Disk Galaxies

S. Callegari, S. Kazantzidis, L. Mayer +4

We perform a suite of high-resolution smoothed particle hydrodynamics simulations to investigate the orbital decay and mass evolution of massive black hole (MBH) pairs down to scal…

astro-ph.CO2009★ 257 cited

Direct Formation of Supermassive Black Holes via Multi-Scale Gas Inflows in Galaxy Mergers

Lucio Mayer, Stelios Kazantzidis, Andres Escala +1

Observations of distant bright quasars suggest that billion solar mass supermassive black holes (SMBHs) were already in place less than a billion years after the Big Bang. Models i…