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- W3120996427 abstract "We analyze a suite of $30$ high resolution zoom-in cosmological hydrodynamic simulations of massive galaxies with stellar masses $M_{ast} > 10^{10.9} M_odot$, with the goal of better understanding merger activity in AGN, AGN activity in merging systems, SMBH growth during mergers, and the role of gas content. Using the radiative transfer code textsc{Powderday}, we generate HST-WFC3 F160W synthetic observations of redshift $0.5 10^{45}$ erg s$^{-1})$ AGN in our sample are no more likely than inactive galaxies $(L_{rm bol} $1:4) do not necessarily enhance AGN activity or significantly grow the central SMBH. We conclude that in the simulated massive galaxies studied here, mergers are not the primary drivers of AGN." @default.
- W3120996427 created "2021-01-18" @default.
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- W3120996427 date "2021-01-05" @default.
- W3120996427 modified "2023-10-18" @default.
- W3120996427 title "The Connection between Mergers and AGN Activity in Simulated and Observed Massive Galaxies" @default.
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