Citizen science discovery of a bow-and-arrow radio galaxy with ~560 kpc bow-shock-like structure in a multi-halo environment at z=0.159.
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5 Pith papers cite this work. Polarity classification is still indexing.
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New ASKAP continuum imaging classifies jet morphologies in 173 G4Jy-3CRE sources (66% of sample) including 37 newly detected jets and identifies six new optical counterparts.
High magnetization and flickering variability in relativistic MHD simulations create asymmetrical cocoons and broken jet morphologies in AGN jets.
Fornax cluster magnetic field follows a power-law spectrum of slope ~2.7 with central strength ~5 μG scaling as n^1.6, consistent with recent central re-amplification and trends across 17 clusters.
The work proposes GRMHD jet simulations to generate synthetic synchrotron maps and polarization signatures for testing physical models of observed magnetic filaments.
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The impact of flickering variability and magnetisation on the dynamics, stability and morphology of radio-loud AGN jets
High magnetization and flickering variability in relativistic MHD simulations create asymmetrical cocoons and broken jet morphologies in AGN jets.