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Using Hα Filaments to Probe Active Galactic Nuclei Feedback in Galaxy Clusters
2019
Astrophysical Journal Letters
Recent observations of giant ellipticals and brightest cluster galaxies (BCGs) provide tentative evidence for a correlation between the luminosity of the Hα emitting gas filaments and the strength of feedback associated with the active galactic nucleus (AGN). Motivated by this, we use 3D radiation-hydrodynamic simulations with the code Enzo to examine and quantify the relationship between the observable properties of the Hα filaments and the kinetic and radiative feedback from supermassive
doi:10.3847/2041-8213/ab0375
fatcat:rjtjvzlh5rccjliatbbrziv6re