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The distribution of radio quiet active galactic nuclei in the star formation-stellar mass plane

That active galactic nuclei (AGN) with jets can alternately enhance as well as suppress star formation rates, explains the location and slope of radio loud AGN on the star formation rate-stellar mass plane. Here, we explore 860 type 1 and 2 AGN at z<0.2 from the ROSAT-2XRS survey in order to understand both different location and lower slopes for non-jetted AGN in the star formation rate-stellar mass plane. We describe the nature of these differences in terms of different degrees of black hole feedback, with relatively weak negative feedback from non-jetted AGN compared to both relatively strong positive and negative feedback from jetted AGN. The validity of these ideas brings us a step closer towards understanding the black hole scaling relation across space and time.

preprint2022arXivOpen access
D. GarofaloG. Mountrichas
astro-ph.GA
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Open access2 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
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D. GarofaloG. Mountrichas

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