Radio-AGN Feedback: When the Little Ones were Monsters

W. L. Williams, H. J. A. Röttgering

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    We present a study of the evolution of the fraction of radio-loud active galactic nuclei (AGN) as a function of their host stellar mass. We make use of two samples of radio galaxies: one in the local universe, $0.01 10^{24}$ W/Hz at z ~ 1-2 while the radio-loud fraction for higher mass galaxies ($M_* > 10^{11.25}$ M$_{\odot}$) remains the same. We argue that this increase is driven largely by the increase in cold or radiative mode accretion with increasing cold gas supply at earlier epochs. The increasing population of low mass Radio-Loud AGN can thus explain the upturn in the Radio Luminosity Function (RLF) at high redshift which is important for understanding the impact of AGN feedback in galaxy evolution.
    Original languageEnglish
    Pages (from-to)1538-1545
    Number of pages8
    JournalMonthly Notices of the Royal Astronomical Society
    Issue number2
    Early online date25 Apr 2015
    Publication statusPublished - 21 Jun 2015


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