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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 5.

Total cold gas mass per halo, Mcg (in M) vs. the number of massive (M* > 108 M) satellites in a halo. The left, middle, and right panels show log M*C = 10.160–10.405, log M*C = 10.453–10.715, and log M*C = 10.931–11.288 bin halos. As in Figure 3, respective quartiles and 1σ ranges are marked. Note that, in the highest-mass bin, the median satellite-rich quartile, ranked according to Nsats (dark green cross), exactly overlaps with the corresponding median ranked according to the number of massive satellites (black cross).

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