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(1 - 6 of 6)
EVN observations of 6.7 GHz methanol maser polarization in massive star-forming regions. V. Completion of the flux-limited sample
Magnetic field strength in cosmic web filaments
The redshift evolution of extragalactic magnetic fields
Constraints on the magnetic field structure in accreting compact objects from aperiodic variability
Losing a minute every two years
The link between turbulence, magnetic fields, filaments, and star formation in the central molecular zone cloud G0,253+0.016