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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 3.

Total cold gas mass per halo, Mcg, (in M) vs. total mass in all satellite galaxies per halo, Mtms (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 2, the numbers of satellite-based medians (﹩{\bar{N}}_{\mathrm{sats}}﹩) are represented by colored cross symbols. Mtms-based median values (﹩{\bar{M}}_{\mathrm{tms}}﹩) are shown as light gray, gray, and black crosses, respectively.

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