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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 4.

Total cold gas mass per halo, Mcg, (in M) vs. the stellar mass of the most massive satellite galaxy in each halo, M*mms (in M) for CGM+Satellites (top panels) and CGM-Satellites (bottom panels) for the log M*C = 10.160–10.405 (left panels), log M*C = 10.453–10.715 (middle panels), and log M*C = 10.931–11.288 (right panels) bin halos. As in Figure 3, respective quartiles and 1σ ranges are marked.

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