On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
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Abstract
In this paper we investigate how massive central galaxies cease their star
formation by comparing theoretical predictions from cosmological simulations:
EAGLE, Illustris and IllustrisTNG with observations of the local Universe from
the Sloan Digital Sky Survey (SDSS). Our machine learning (ML) classification
reveals supermassive black hole mass (
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1365-2966
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Foundation MERAC (Mobilising European Research in Astrophysics and Cosmology) (Unknown)
STFC (ST/V000918/1)
Royal Society (RSRP\R1\211056)