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Using Hα Filaments to Probe Active Galactic Nuclei Feedback in Galaxy Clusters

  • Authors: Yu Qiu, Tamara Bogdanović, Yuan Li, and Michael McDonald

2019 The Astrophysical Journal Letters 872 L11.

  • Provider: AAS Journals

Caption: Figure 2.

Left panel: evolution of the average kinetic (blue triangles), radiative luminosity (black circles), and Hα filament mass (multicolor stars) measured in simulation RT02. Right panel: the kinetic (multicolor triangle) and radiative (black circle) luminosity as a function of the filament mass. The color marks the time in the simulation. Correlation of ﹩\langle {L}_{{\rm{K}}}\rangle ﹩ (﹩\langle {L}_{{\rm{R}}}\rangle ﹩) with the Hα filament mass for the first 9 Gyr is represented by the solid black (dashed blue) line.

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