Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …

MeerKAT's large number (64) of 13.5 m diameter antennas, spanning 8 km with a densely
packed 1 km core, create a powerful instrument for wide-area surveys, with high sensitivity …

Thin synchrotron-emitting filaments are increasingly seen in the intracluster medium (ICM).
We present the first example of a direct interaction between a magnetic filament, a radio jet …

We have examined the distribution of the position angle (PA) of the Galactic center filaments
with lengths L> 66''and< 66''as well as their length distribution as a function of PA. We find …

Giant radio sources (GRSs) defined to be> 0.7 Mpc are the largest single objects in the
Universe and can be associated with both galaxies (GRGs) and quasars (GRQs). They are …

We present the full panchromatic afterglow light-curve data of GW170817, including new
radio data as well as archival optical and X-ray data, between 0.5 and 940 days post …

Jets from active galactic nuclei (AGN) are known to recurrently enrich their surrounding
medium with mildly relativistic particles and magnetic fields. Here, we present a detailed …

We introduce the first AI-based framework for deep, super-resolution, wide-field radio
interferometric imaging and demonstrate it on observations of the ESO 137-006 radio …

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 …

Context. Dynamical motions in the intra-cluster medium (ICM) can imprint distinctive features
on X-ray images that map the thermal bremsstrahlung emission from galaxy clusters, such …