DD.3.01 — Towards an understanding of the Radio-mode AGN Feedback at higher redshifts

Date & Time

Aug 7th at 4:00 PM until 4:30 PM




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Author(s): Laura Bîrzan1

Institution(s): 1. Leiden Observatory

Direct evidence for feedback by active galactic nuclei (AGN) on the intra-cluster medium (ICM) of nearby groups and clusters has been provided by Chandra X-ray images. They show that the radio lobes emitted by the AGN create cavities in the hot cluster atmosphere, which
affects the cooling gas that leads to star formation and galaxy growth and allow a direct measurement of the bulk of the AGN's power. Consequently, AGN feedback is now recognized as a necessary ingredient for galaxy formation models to prevent overcooling in massive halos. It is therefore important to study AGN feedback at redshifts where clusters are known to form (z ~ 1) and AGN feedback is predicted to regulate star formation in the most massive galaxies. Together with radio data, the cavities allow us to derive scaling relations that can be used to estimate the AGN feedback power using only radio data. I will review the importance of such relations for extending current studies of feedback with new and upcoming radio telescopes such as LOFAR and SKA, and I will present preliminary results from deep low-frequency LOFAR observations of the NEP field to understand if the local cooling-to-heating balance and the corresponding scaling relations (between jet power and radio luminosity) hold at these redshifts (z > 0.5).