Using Chandra X-ray and Very Large Array radio data, we investigate the scaling
relationship between jet power, P jet, and synchrotron luminosity, P radio. We expand the …

The MeerKAT Fornax Survey maps the distribution and kinematics of atomic neutral
hydrogen gas (HI) in the nearby Fornax galaxy cluster using the MeerKAT telescope. The 12 …

We present the first subarcsecond-resolution mid-infrared (MIR) atlas of local active galactic
nuclei (AGN). Our atlas contains 253 AGN with a median redshift of z= 0.016, and includes …

Taking advantage of the unprecedented combination of sensitivity and angular resolution
afforded by the Herschel Space Observatory at far-infrared and submillimetre wavelengths …

We present a multi-wavelength study of the gaseous medium surrounding the nearby active
galactic nucleus (AGN), Fornax A. Using MeerKAT, ALMA, and MUSE observations, we …

The origin of ultrahigh energy cosmic rays (UHECRs) has been an open question for
decades. Here, we use a combination of hydrodynamic simulations and general physical …

As part of the Fornax Deep Survey with the ESO VLT Survey Telescope, we present new g-
and r-band mosaics of the SW group of the Fornax Cluster. It covers an area of 3× 2 square …

We study the recent star formation histories of 10 galaxies in the Fornax A galaxy group, on
the outskirts of the Fornax cluster. The group galaxies are gas-rich, and their neutral atomic …

The origin of ultrahigh energy cosmic rays (UHECRs) is still unknown. It has recently been
proposed that UHECR anisotropies can be attributed to starburst galaxies or active galactic …

Many massive early-type galaxies host central radio sources and hot X-ray atmospheres
indicating the presence of radio-mechanical active galactic nucleus (AGN) feedback. The …