Activity restart - a key to explaining the morphology of J1211+743

TL;DR

This paper proposes that the asymmetric morphology of the giant radio galaxy J1211+743 can be explained by a re-ignition of activity in its nucleus, with the observed features resulting from an activity switch-off and orientation effects.

Contribution

It introduces a novel activity restart model to explain the complex lobe and jet asymmetries in J1211+743, challenging standard double-lobed source paradigms.

Findings

The relic lobe is on the near side, explaining its lack of a hotspot.

The jet points towards the relic lobe, consistent with a recent activity phase.

Orientation and activity switch-off account for lobe asymmetries.

Abstract

J1211+743 is a giant radio galaxy with a one-sided jet and two asymmetric lobes, one of which is of Fanaroff-Riley (FR) type II with a hotspot and the other is a diffuse relic devoid of a hotspot. The jet points towards the latter lobe, which is difficult to explain in a standard way within the double-lobed radio source paradigm. Here, I propose to assume that the nucleus of J1211+743 has undergone a re-ignition of activity and its lobes, presumably both originally of FR II type, represent an earlier active phase, while the jet represents the current one. The asymmetry of the lobes is a consequence of the orientation of the source combined with an activity switch-off that occurred between two active periods. The relic lobe is on the near side with regard to the observer, whereas the radiation from the far-side lobe arrives significantly later owing to its longer distance to the observer. The far-side lobe is thus perceived to have not yet decayed. On the other hand, the jet behaves in a standard way, i.e. its projected orientation reflects the near side of the source. Hence, we are able to explain why the location of the relic lobe correlates with the direction of the jet.