activity
20002025
most citedStreaming Motions Towards the Supermassive Black Hole in NGC 1097

111 citations · 396 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.GA2025

The quest for high-redshift radio galaxies. I. A pilot spectroscopic study

Alessandro Capetti, Barbara Balmaverde, Miguel Coloma Puga +4

The population of high-redshift radio galaxies (HzRGs) is still poorly studied because only a few of these objects are currently known. We here present the results of a pilot proje…

astro-ph.GA2025

A recoiling supermassive black hole in a powerful quasar

Marco Chiaberge, Takahiro Morishita, Matteo Boschini +14

Supermassive black holes (SMBH) are thought to grow through accretion of matter and mergers. Models of SMBH mergers have long suffered the final parsec problem, where SMBH binaries…

astro-ph.GA2024

The radio properties of z>3.5 quasars: Are most high-redshift radio-loud active galactic nuclei obscured?

Alessandro Capetti, Barbara Balmaverde

We explore the radio properties of powerful (rest-frame luminosity W Hz at 500 MHz) high-redshift (z > 3.5) quasars. The aim of this study is to gain a bett…

astro-ph.GA2024

The large-scale environment of 3CR radio galaxies at z<0.3

Samantha Casadei, Alessandro Capetti, Claudia M. Raiteri +1

The question of whether and how the properties of radio galaxies (RGs) are connected with the large-scale environment is still an open issue. For this work we measured the large-sc…

astro-ph.HE2024

The different flavors of extragalactic jets: Magnetized relativistic flows

Paola Rossi, Gianluigi Bodo, Silvano Massaglia +1

We perform three-dimensional numerical simulations of magnetized relativistic jets propagating in a uniform density environment in order to study the effect of the entrainment and…

astro-ph.HE2024★ 1 cited

FR0 jets and recollimation-induced instabilities

A. Costa, G. Bodo, F. Tavecchio +6

The recently discovered population of faint FR0 radiogalaxies has been interpreted as the extension to low power of the classical FRI sources. Their radio emission appears to be co…