activity
20072026
most citedBlack holes, gravitational waves and fundamental physics: a roadmap

742 citations · 2.9k across the 72 of their papers we have counts for

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Showing 2016Show all

5 papers · 1 filter

astro-ph.GA2016★ 40 cited

Galactic angular momentum in cosmological zoom-in simulations. I. Disk and bulge components and the galaxy--halo connection

Aleksandra Sokolowska, Pedro R. Capelo, S. Michael Fall +3

We investigate the angular momentum evolution of four disk galaxies residing in Milky Way-sized halos formed in cosmological zoom-in simulations with various sub-grid physics and m…

astro-ph.GA2016★ 78 cited

Shocks and angular momentum flips: a different path to feeding the nuclear regions of merging galaxies

Pedro R. Capelo, Massimo Dotti

We study the dynamics of galaxy mergers, with emphasis on the gas feeding of nuclear regions, using a suite of hydrodynamical simulations of galaxy encounters. The high spatial and…

astro-ph.GA2016★ 101 cited

A survey of dual active galactic nuclei in simulations of galaxy mergers: frequency and properties

Pedro R. Capelo, Massimo Dotti, Marta Volonteri +3

We investigate the simultaneous triggering of active galactic nuclei (AGN) in merging galaxies, using a large suite of high-resolution hydrodynamical simulations. We compute dual-A…

astro-ph.GA2016★ 59 cited

The Pairing of Accreting Massive Black Holes in Multiphase Circumnuclear Disks: the Interplay between Radiative Cooling, Star Formation, and Feedback Processes

Rafael Souza Lima, Lucio Mayer, Pedro R. Capelo +1

We study the orbital decay of a pair of massive black holes (BHs) with masses 5 * 10^5 and 10^7 M_sun, using hydrodynamical simulations of circumnuclear disks (CNDs) with the alter…

astro-ph.GA2016★ 63 cited

Supermassive black hole pairs in clumpy galaxies at high redshift: delayed binary formation and concurrent mass growth

Valentina Tamburello, Pedro R. Capelo, Lucio Mayer +2

Massive gas-rich galaxy discs at host massive star-forming clumps with typical baryonic masses in the range ~M which can affect the orbital decay…