Compact steep-spectrum (CSS) and peaked-spectrum (PS) radio sources are compact,
powerful radio sources. The multi-frequency observational properties and current theories …

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 …

The morphological classification of radio sources is important to gain a full understanding of
galaxy evolution processes and their relation with local environmental properties …

What determines the nuclear radio emission in local galaxies? To address this question, we
combine optical [O iii] line emission, robust black hole (BH) mass estimates, and high …

Context. The local radio-loud AGN population is dominated by compact sources named
FR0s. These sources show features, for example the host type, the mass of the …

We have carried out relativistic three-dimensional simulations of high-power radio sources
propagating i, nto asymmetric cluster environments. We offset the environment by 0 or 1 core …

We explore the low-frequency radio properties of the sources in the Fanaroff-Riley class 0
catalog (FR0CAT) as seen by the Low-Frequency ARray (LOFAR) observations at 150 MHz …

We report the high-resolution radio observations of eight Fanaroff–Riley type 0 radio
galaxies (FR 0s), selected from the published FR 0 sample. These observations were …

In the espresso scenario, ultra-high-energy (UHE) cosmic rays (CRs) are produced via a
one-shot reacceleration of galactic-like CRs in the relativistic jets of active galactic nuclei …

We present the first X-ray dedicated study of the galaxy cluster Abell 795 (A795) and of the
Fanaroff–Riley type 0 (FR0) hosted in its brightest cluster galaxy. Using an archival 30 ks …