Jetted subgalactic-size radio sources in merging galaxies -- A jet redirection scenario

TL;DR

This paper proposes that rapid jet redirection caused by precession or orbital motion in merging galaxies explains why many subgalactic-size radio sources remain confined and do not evolve into larger radio galaxies.

Contribution

It introduces a jet redirection scenario driven by galaxy mergers to explain the properties and prevalence of jetted subgalactic-size radio sources.

Findings

Many sources show transverse motion consistent with jet precession.

Radio morphologies suggest presence of large-angle, short-period precessing jets.

Most sources are in merging systems at different evolutionary stages.

Abstract

Context: The long-standing question concerning jetted subgalactic-size (JSS) radio sources is whether they will evolve into large radio galaxies, die before escaping the host galaxy, or remain indefinitely confined to their compact size. Aims: Our main goal is to propose a scenario that explains the relative number of JSS radio sources and their general properties. Methods: We studied the parsec-scale radio morphology of a complete sample of 21 objects using Very Long Baseline Array (VLBA) observations at various frequencies and analyzed the morphological characteristics of their optical hosts. Results: Many of these radio sources exhibit radio morphologies consistent with transverse motions of their bright edges and are found in dynamically disturbed galaxies. VLBA images suggest the possible presence of large-angle, short-period precessing jets, and an orbital motion of the radio-loud active galactic nucleus (AGN) in a dual or binary system. The majority of JSS radio sources appear to be in systems in different stages of their merging evolution. Conclusions: We propose a scenario where rapid jet redirection, through precession or orbital motion, prevents the jet from penetrating the interstellar medium (ISM) sufficiently to escape the host galaxy. Most JSS radio sources remain compact due to their occurrence in merging galaxies.