6–10 May 2024
Bologna, Italy
Europe/Rome timezone

The nature of compact radio-loud AGN: a systematic look at the LOFAR AGN population

9 May 2024, 11:45
15m
Bologna, Italy

Bologna, Italy

Speaker

Jones Chilufya (University of Hertfordshire)

Description

The advent of long-baseline interferometers such as the LOw-Frequency Array (LOFAR) telescope enables high angular resolution and sensitivity, which is crucial for understanding synchrotron emission processes and the low-frequency spectral behaviour of radio-loud active galactic nuclei (RLAGN). Using the large RLAGN sample constructed from the LOFAR Two-metre Sky Survey (LoTSS) first data release, we have selected 55 candidates of unresolved high-excitation radio galaxies to investigate the nature of an emerging population of low-luminosity compact RLAGN numerically dominating the local Universe on sub-kpc scales. These objects are unresolved at 6 arcsec angular resolution at 150 MHz. We use high-frequency 6 GHz Very Large Array (VLA) observations of these sources to resolve them on the sub-kpc scale. We show that many of these objects remain compact at 0.3 arcsec angular resolution, which corresponds to an upper limit of less than 1 kpc in physical size, whereas a small fraction of sources shows sub-kpc extended radio emission. The latter exhibit varied radio morphologies including double-lobed, one-sided, and two-sided structures. The radio spectra of our sample computed between 150 MHz and 6 GHz range from steep to flat/inverted and span the range seen for various sources such as compact symmetric objects, compact steep-spectrum sources, and gigahertz-peaked spectrum sources. We investigate the environments in and around these compact objects using synchrotron self-absorption and free-free absorption models and find that the former is the likely explanation of the spectral turnover observed in some sources at 150 MHz. Using the power/linear size diagram, we speculate that our objects, in terms of luminosity, could represent a continuity between Seyferts and radio-quiet quasars in AGN unified models. A comparison with so-called FR0 sources indicate that they could be drawn from the same spectral index distribution and share similar radio-powers and morphologies.

In-person or online? in-person
keywords galaxies: jets − galaxies: active − radio continuum: galaxies
Career level Student

Primary authors

Jones Chilufya (University of Hertfordshire) Prof. Martin Hardcastle (University of Hertfordshire) Dr Jonathon Pierce (University of Hertfordshire) Dr Judith Croston (The Open University) Dr Beatriz Mingo (The Open University) Dr Xuechen Zheng (Leiden University) Dr Ranieri Baldi (INAF - Instituto di Radioastronomia) Prof. Huub Röttgering (Leiden University)

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