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Searching for Correlations between Satellite Galaxy Populations and the Cold Circumgalactic Medium around TNG50 Galaxies

  • Authors: Mitali Damle, Stephanie Tonnesen, Martin Sparre, Philipp Richter

Mitali Damle et al 2025 The Astrophysical Journal 986 .

  • Provider: AAS Journals

Caption: Figure A1.

Scatter plots for the low-mass bin (log M*C = 10.160–10.405) halos probing correlations between the number of satellite galaxies per halo (Nsats), M*, M*C, M200c, Mgas, Mcg, Mbh (all in log M), and SFR (in M yr−1). The 25th (Satellite-poor), 50th, and 75th (Satellite-rich) quartiles are shown as aqua, blue, and teal points, respectively. Histograms for the satellite-poor and satellite-rich quartiles for corresponding halo attributes are also shown in the form of blue and orange bars, respectively.

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