Gamma-ray emission in radio galaxies under the VLBI scope: I. Parsec-scale jet kinematics and high-energy properties of Y-ray-detected TANAMI radio galaxies

Aims . In the framework of the multi-wavelength and very long baseline interferometry (VLBI) monitoring program TANAMI (Tracking Active Nuclei with Austral Milliarcsecond Interferometry), we study the evolution of the parsec-scale radio emission in radio galaxies in the southern hemisphere and their...

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Bibliographic Details
Published in:Astronomy & Astrophysics
Main Authors: Angioni, R, Ros, E, Kadler, M, Ojha, R, Mueller, C, Edwards, PG, Burd, PR, Carpenter, B, Dutka, MS, Gulyaev, S, Hase, H, Horiuchi, S, Krauss, F, Lovell, JEJ, Natusch, T, Phillips, C, Ploetz, C, Quick, JFH, Roesch, F, Schulz, R, Stevens, J, Tzioumis, AK, Weston, S, Wilms, J, Zensus, JA
Format: Article in Journal/Newspaper
Language:English
Published: EDP Sciences 2019
Subjects:
Physical Sciences
Astronomical sciences
Galactic astronomy
Austral
New Zealand
Riley
The ''Y''
Antarc*
Antarctica
Online Access:https://doi.org/10.1051/0004-6361/201935697
http://ecite.utas.edu.au/152736
Description
Summary:Aims . In the framework of the multi-wavelength and very long baseline interferometry (VLBI) monitoring program TANAMI (Tracking Active Nuclei with Austral Milliarcsecond Interferometry), we study the evolution of the parsec-scale radio emission in radio galaxies in the southern hemisphere and their relationship to the Y -ray properties of the sources. Our study investigates systematically, for the first time, the relationship between the two energy regimes in radio galaxies. In this first paper, we focus on Fermi -LAT-detected sources. Methods . The TANAMI program monitors a large sample of radio-loud AGN at 8.4 GHz and 22.3 GHz with the Australian long baseline array (LBA) and associated telescopes in Antarctica, Chile, New Zealand and South Africa. We performed a kinematic analysis for five Y -ray detected radio galaxies using multi-epoch 8.4 GHz VLBI images, deriving limits on intrinsic jet parameters such as speed and viewing angle. We analyzed 103 months of Fermi -LAT data in order to study possible connections between the Y -ray properties and the pc-scale jets of Fermi -LAT-detected radio galaxies, both in terms of variability and average properties. We discuss the individual source results and draw preliminary conclusions on sample properties including published VLBI results from the MOJAVE (Monitoring Of Jets in Active galactic nuclei with VLBA Experiments) survey, with a total of fifteen sources. Results . We find that the first Y -ray detection of Pictor A might be associated with the passage of a new VLBI component through the radio core, which appears to be a defining feature of high-energy emitting Fanaroff-Riley type II radio galaxies. We detect subluminal parsec-scale jet motions in the peculiar AGN PKS 0521-36, and we confirm the presence of fast Y -ray variability in the source down to timescales of six hours, which is not accompanied by variations in the VLBI jet. We robustly confirm the presence of significant superluminal motion, up to B app ~3, in the jet of the TeV radio galaxy PKS ...

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