Research news on Radio galaxies

Radio galaxies as a research area focus on extragalactic systems whose active galactic nuclei and associated relativistic jets emit strongly at radio wavelengths, often dominating their bolometric output. This field encompasses the physics of jet launching and collimation from accreting supermassive black holes, particle acceleration, synchrotron and inverse-Compton emission processes, and the interaction of jets and radio lobes with the interstellar and intracluster medium. Research on radio galaxies is central to understanding AGN feedback in galaxy formation and evolution, environmental dependence of radio-loud activity, large-scale magnetic fields, and the use of radio-loud AGN as probes of cosmology and large-scale structure.

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 ...

Exploring the hidden rings of the Milky Way

Radio astronomy opens a window onto the invisible universe. While our eyes can detect visible light, countless objects in space emit radiation at much longer wavelengths, in the radio portion of the electromagnetic spectrum. ...

page 1 from 2