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The Baryonic Mass–Halo Mass Relation of Extragalactic Systems

  • Authors: Stacy S. McGaugh, Tobias Mistele, Francis Duey, Konstantin Haubner, Federico Lelli, James M. Schombert, Pengfei Li

Stacy S. McGaugh et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 5.

The baryonic mass fraction as a function of mass M200 with the equivalent V200 noted on the top axis. Data and symbols are the same as in Figures 2 and 3. The top panels follow from using rotation curve fits to estimate halo mass as in Figure 2 for pseudo-isothermal (top-left panel) and NFW (top-right panel) halo models. The bottom panels follow from using the flat rotation speed as the halo mass estimator as in Figure 3 with fv = 1.0 (bottom-left panel) or fv = 1.4 (bottom-right panel) for the kinematic data; the lensing data are unchanged.

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