M87's giant radio lobes are continuously refilled AGN outflows with an age of about 30-50 Myr, requiring (0.2-2) x 10^44 erg/s for the diffuse component and (1-11) x 10^44 erg/s for the whole source.
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MWA and VLA Observations of Diffuse Radio Lobes in M 87
M87's giant radio lobes are continuously refilled AGN outflows with an age of about 30-50 Myr, requiring (0.2-2) x 10^44 erg/s for the diffuse component and (1-11) x 10^44 erg/s for the whole source.