activity
19992026
most citedClusters of galaxies : observational properties of the diffuse radio emission

644 citations · 5.6k across the 94 of their papers we have counts for

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Showing 2017Show all

6 papers · 1 filter

astro-ph.GA2017★ 19 cited

Studying the late evolution of a radio-loud AGN in a galaxy group with LOFAR

Federica Savini, Annalisa Bonafede, Marcus Brüggen +17

Feedback by radio-loud active galactic nuclei (AGN) in galaxy groups is not fully understood. Open questions include the duty cycle of the AGN, the spatial extent of the radio lobe…

astro-ph.GA2017

The MeerKAT Fornax Survey

P. Serra, W. J. G. de Blok, G. L. Bryan +18

We present the science case and observations plan of the MeerKAT Fornax Survey, an HI and radio continuum survey of the Fornax galaxy cluster to be carried out with the SKA precurs…

astro-ph.GA2017★ 29 cited

Narrow head-tail radio galaxies at very high resolution

Beatrice Terni de Gregory, Luigina Feretti, Gabriele Giovannini +4

Aims. Narrow-angle tailed (NAT) sources in clusters of galaxies can show on the large scale very narrow tails that are unresolved even at arcsecond resolution. These sources could…

astro-ph.CO2017★ 31 cited

Observations of the galaxy cluster CIZA J2242.8+5301 with the Sardinia Radio Telescope

F. Loi, M. Murgia, F. Govoni +25

We observed the galaxy cluster CIZA J2242.8+5301 with the Sardinia Radio Telescope to provide new constraints on its spectral properties at high frequency. We conducted observation…

astro-ph.GA2017★ 90 cited

Search and modelling of remnant radio galaxies in the LOFAR Lockman Hole field

M. Brienza, L. Godfrey, R. Morganti +8

The phase of radio galaxy evolution after the jets have switched off, often referred to as the remnant phase, is poorly understood and very few sources in this phase are known. In…

astro-ph.GA2017★ 48 cited

Radiative age mapping of the remnant radio galaxy B2 0924+30: the LOFAR perspective

A. Shulevski, R. Morganti, J. J. Harwood +9

We have observed the steep spectrum radio source B2 0924+30 using the LOw Frequency ARray (LOFAR) telescope. Hosted by a z=0.026 elliptical galaxy, it has a relatively large angula…