Radio-loud compact radio sources (CRSs) are characterised by morphological compactness
of the jet structure centred on the active nucleus of the galaxy. Most of the local elliptical …

Despite their relative sparseness, during the recent years it has become more and more
clear that extragalactic radio sources (both AGN and star-forming galaxies) constitute an …

Associated with one of the most important forms of active galactic nucleus (AGN) feedback,
and showing a strong preference for giant elliptical host galaxies, radio AGN (L_ 1.4\, GHz> …

Radio-loud active galaxies have two accretion modes [radiatively inefficient (RI) and
radiatively efficient (RE)], with distinct optical and infrared signatures, and two jet dynamical …

We present the results of a pilot JVLA project aimed at studying the bulk of the radio-emitting
AGN population, that was unveiled by the NVSS/FIRST and SDSS surveys. The key …

We present the first data release of high-resolution (≤ 0.2 arcsec) 1.5-GHz radio images of
103 nearby galaxies from the Palomar sample, observed with the eMERLIN array, as part of …

The M 6 109×⊙ supermassive black hole at the center of the giant elliptical galaxy M87
powers a relativistic jet. Observations at millimeter wavelengths with the Event Horizon …

Aims. The radio galaxy NGC 1275, recently identified as a very high energy (VHE,> 100
GeV) γ-ray emitter by MAGIC, is one of the few non-blazar active galactic nuclei detected in …

We discuss the γ-ray emission of the radiogalaxy NGC 1275 (the central galaxy of the
Perseus Cluster), detected by Fermi-LAT (very-high energies) and MAGIC, in the framework …

The coalescence of a binary black hole can be accompanied by a large gravitational recoil
due to anisotropic emission of gravitational waves. A recoiling supermassive black hole …