Fig. 7.
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Cumulative mass of the hot gas as a function of the distance from the Galactic center r. For the combined (β ≡ 0.5) model, the solid and dashed lines respectively show the spherical and disk-like components. The horizontal gray lines show 10%, 30%, and 100% of fb × 1012 M⊙, where fb ≡ Σb/Σm = 0.071 is the cosmic baryon fraction.
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