Feedback factory : multiple faint radio jets detected in a cluster at z=2

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http://hdl.handle.net/10138/330287

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Kalita , B S , Daddi , E , Coogan , R T , Delvecchio , I , Gobat , R , Valentino , F , Strazzullo , V , Tremou , E , Gomez-Guijarro , C , Elbaz , D & Finoguenov , A 2021 , ' Feedback factory : multiple faint radio jets detected in a cluster at z=2 ' , Monthly Notices of the Royal Astronomical Society , vol. 503 , no. 1 , pp. 1174-1186 . https://doi.org/10.1093/mnras/stab559

Title: Feedback factory : multiple faint radio jets detected in a cluster at z=2
Author: Kalita, Boris S.; Daddi, Emanuele; Coogan, Rosemary T.; Delvecchio, Ivan; Gobat, Raphael; Valentino, Francesco; Strazzullo, Veronica; Tremou, Evangelia; Gomez-Guijarro, Carlos; Elbaz, David; Finoguenov, Alexis
Contributor: University of Helsinki, Department of Physics
Date: 2021-05
Language: eng
Number of pages: 13
Belongs to series: Monthly Notices of the Royal Astronomical Society
ISSN: 0035-8711
URI: http://hdl.handle.net/10138/330287
Abstract: We report the detection of multiple faint radio sources, that we identify as active galactic nucleus (AGN) jets, within CLJ1449+0856 at z = 2 using 3 GHz Very Large Array observations. We study the effects of radio-jet-based kinetic feedback at high redshifts, which has been found to be crucial in low-redshift clusters to explain the observed thermodynamic properties of their intracluster medium (ICM). We investigate this interaction at an epoch featuring high levels of AGN activity and a transitional phase of ICM in regards to the likelihood of residual cold gas accretion. We measure a total flux of 30.6 +/- 3.3 mu Jy from the six detected jets. Their power contribution is estimated to be 1.2 (+/- 0.6) x 10(44) erg s(-1), although this value could be up to 4.7 x 10(44) erg s(-1). This is a factor of similar to 0.25-1.0 of the previously estimated instantaneous energy injection into the ICM of CLJ1449+0856 from AGN outflows and star formation that have already been found to be sufficient in globally offsetting the cooling flows in the cluster core. In line with the already detected abundance of star formation, this mode of feedback being distributed over multiple sites, contrary to a single central source observed at low redshifts, points to accretion of gas into the cluster centre. This also suggests a 'steady state' of the cluster featuring non-cool-core-like behaviour. Finally, we also examine the total infrared-radio luminosity ratio for the known sample of galaxies within the cluster core and find that dense environments do not have any serious consequence on the compliance of galaxies to the infrared-radio correlation.
Subject: galaxies: active
galaxies: clusters: general
galaxies: evolution
galaxies: high-redshift
radio continuum: galaxies
ACTIVE GALACTIC NUCLEI
STAR-FORMING GALAXIES
GHZ LARGE PROJECT
CL J1449+0856
MOLECULAR GAS
CHANDRA OBSERVATION
GRISM CONFIRMATION
HOST GALAXIES
RAY
AGN
115 Astronomy, Space science
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