Research news on Radio jets

Radio jets as a research area focuses on the formation, propagation, and emission properties of collimated, relativistic outflows from active galactic nuclei, X-ray binaries, and other compact objects, observed primarily at radio wavelengths. This field investigates jet launching mechanisms (e.g., magnetohydrodynamic processes near accreting black holes), particle acceleration, synchrotron and inverse-Compton emission, jet–interstellar/intergalactic medium interactions, and the role of jets in feedback on galaxy and cluster evolution. Research combines high-resolution radio interferometry, multiwavelength observations, numerical simulations, and theoretical modeling to constrain jet composition, energetics, magnetic field structure, and kinematics across different cosmic environments.

Intermittent black hole jets are like a 'cosmic volcano'

When astronomers look out into the cosmos, they see supermassive black holes (SMBH) in two different states. In one state, they're dormant. They're actively accreting only a tiny amount of matter and emit only faint, weak ...

Probing the jet base of M87's supermassive black hole

Some galaxies eject powerful streams of charged particles—jets—from their centers into space. The prominent jet of Messier 87 (M87) in the constellation Virgo is visible over distances of 3,000 light-years and can be observed ...

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