Figure 10 from Correlations between Black Holes and Host Galaxies in the Illustris and IllustrisTNG Simulations

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Correlations between Black Holes and Host Galaxies in the Illustris and IllustrisTNG Simulations

Authors: Yuan Li, Melanie Habouzit, Shy Genel, Rachel Somerville, Bryan A. Terrazas, Eric F. Bell, Annalisa Pillepich, Dylan Nelson, Rainer Weinberger, Vicente Rodriguez-Gomez, Chung-Pei Ma, Ruediger Pakmor, Lars Hernquist, and Mark Vogelsberger

2020 The Astrophysical Journal 895 102.

Provider: AAS Journals

Caption: Figure 10.

Star formation history of low-mass galaxies (σ < 100 km s⁻¹) in TNG100. Colors and lines have the same meanings as Figure 3. Similar to the massive galaxies in TNG100, for low-mass galaxies, the hosts of overmassive SMBHs have higher SFR than the hosts of undermassive SMBHs throughout history, and the normalized star formation histories of the two populations are very similar.

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