A close look at compact triple radio sources
D. Cseh, A. Fuhl, S. Frey

TL;DR
This paper examines the structure of compact triple radio sources, revealing signs of restarted activity and jet reorientation, and discusses the potential for high-resolution VLBI observations to further understand their inner structures.
Contribution
It provides high-resolution imaging evidence of restarted activity and jet reorientation in compact triple radio sources, and identifies candidate quasars for future detailed VLBI studies.
Findings
Inner core structures show signs of restarted activity.
Misalignment between arcsecond and milliarcsecond structures supports jet reorientation.
Two quasars with potential for high-resolution VLBI imaging are identified.
Abstract
We show an archival 1.4-GHz Very Large Array (VLA) image of the core-dominated triple (CDT) radio source J1628+3906, along with a recent high-resolution 5-GHz Very Long Baseline Interferometry (VLBI) image of its core. This core is resolved into two nearly symmetric components at ~10 milli-arcsecond (mas) angular scale. The inner structure is markedly misaligned with respect to the large-scale structure. This morphology can be interpreted as a possible signature of once ceased and then restarted activity of the galactic nucleus, coupled with a rapid repositioning of the central radio jet axis. In a search for compact (<5"), optically identified, and highly redshifted (z>3) quasars in the Faint Images of the Radio Sky at Twenty-centimeters (FIRST) and the Sloan Digital Sky Survey (SDSS) catalogues, we have also found two quasars associated with weaker two-sided radio lobes at ~10" scale.…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology
