Measurements of the quantity of radio-mode feedback injected by an active galactic nucleus
into the cluster environment have mostly relied on X-ray observations, which reveal cavities …

Abstract We present new Atacama Large Millimeter Array observations of the molecular gas
and far-infrared continuum around the brightest cluster galaxy (BCG) in the cool-core cluster …

Brightest cluster galaxies (BCGs) are excellent laboratories for the study of galaxy evolution
in dense Mpc-scale environments. We used the IRAM-30 m to observe, in CO (1→ 0), CO …

Radio mini-halos are clouds of diffuse, low-surface brightness synchrotron emission that
surround the Brightest Cluster Galaxy (BCG) in massive cool-core galaxy clusters. In this …

Context. Low luminosity radio galaxies (LLRGs) typically reside in dense megaparsec-scale
environments and are often associated with brightest cluster galaxies (BCGs). They are an …

We present a search for nuclear X-ray emission in the brightest cluster galaxies (BCGs) of a
sample of groups and clusters of galaxies extracted from the Chandra archive. The exquisite …

Context. The study of substructure is an important step in determining how galaxy clusters
form. Aims. We aim to gain new insights into the controversial dynamical status of MACS …

We set the stage for reassessing how star formation, emission-line nebulae, and active
galactic nuclei (AGNs) in brightest cluster galaxies (BCGs) depend on the thermodynamics …

Aims. Non-thermal properties of galaxy clusters have been studied using detailed and deep
radio images in comparison with X-ray data. While much progress has been made in this …

The mechanisms governing the stellar mass assembly and star formation history of brightest
cluster galaxies (BCGs) are still being debated. By means of new and archival molecular …