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.
Monthly Notices of the Royal Astronomical Society , volume =
4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
years
2026 4verdicts
UNVERDICTED 4representative citing papers
MHD simulations forecast polarized synchrotron emission in clusters and filaments to assess SKA detection capabilities.
Predictions show the SKA-mid RM grid will deliver higher precision and accuracy for intra-cluster and intra-group magnetic field studies than POSSUM.
A review of Faraday Rotation Measure Synthesis techniques and SKA Array Assembly stages for high-resolution Faraday tomography of cosmic magnetic structures.
citing papers explorer
-
The MeerKAT Fornax Survey VII. Characterisation of the Fornax cluster's magnetic field and new insights on magnetisation in large scale systems
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.
-
Study of Polarized Emission in Radio Halos and Filaments in the SKA Telescopes Era
MHD simulations forecast polarized synchrotron emission in clusters and filaments to assess SKA detection capabilities.
-
The Impact of Dense RM Grids on the Study of Intra-cluster and Intra-group Magnetic Fields
Predictions show the SKA-mid RM grid will deliver higher precision and accuracy for intra-cluster and intra-group magnetic field studies than POSSUM.
-
Faraday Tomography with the SKA: A New Era of Cosmic Magnetism Studies
A review of Faraday Rotation Measure Synthesis techniques and SKA Array Assembly stages for high-resolution Faraday tomography of cosmic magnetic structures.