activity
20042022
most citedA radio ridge connecting two galaxy clusters in a filament of the cosmic web

163 citations · 730 across the 12 of their papers we have counts for

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Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2021

Combining LOFAR and Apertif Data for Understanding the Life Cycle of Radio Galaxies

Raffaella Morganti, Nika Jurlin, Tom Oosterloo +10

Active galactic nuclei (AGN) at the centres of galaxies can cycle between periods of activity and of quiescence. Characterising the duty-cycle of AGN is crucial for understanding t…

astro-ph.GA202169 cited

LOFAR imaging of Cygnus A -- Direct detection of a turnover in the hotspot radio spectra

J. P. McKean, L. E. H. Godfrey, S. Vegetti +75

The low-frequency radio spectra of the hotspots within powerful radio galaxies can provide valuable information about the physical processes operating at the site of the jet termin…

astro-ph.GA20209 cited

Extreme intra-hour variability of the radio source J1402+5347 discovered with Apertif

T. A. Oosterloo, H. K. Vedantham, A. M. Kutkin +27

The propagation of radio waves from distant compact radio sources through turbulent interstellar plasma in our Galaxy causes these sources to twinkle, a phenomenon called interstel…

astro-ph.GA202017 cited

Low-frequency observations of the Giant Radio Galaxy NGC 6251

T. M. Cantwell, J. D. Bray, J. H. Croston +22

We present LOFAR observations at 150 MHz of the borderline FRI/FRII giant radio galaxy NGC 6251. This paper presents the most sensitive and highest-resolution images of NGC 6251 at…

astro-ph.GA2019163 cited

A radio ridge connecting two galaxy clusters in a filament of the cosmic web

F. Govoni, E. Orrù, A. Bonafede +26

Galaxy clusters are the most massive gravitationally bound structures in the Universe. They grow by accreting smaller structures in a merging process that produces shocks and turbu…

astro-ph.GA2018

LOFAR MSSS: Flattening low-frequency radio continuum spectra of nearby galaxies

K. T. Chyży, W. Jurusik, J. Piotrowska +35

The shape of low-frequency radio continuum spectra of normal galaxies is not well understood, the key question being the role of physical processes such as thermal absorption in sh…