Fig. 1.
Maximum particle density of the hydrostatic halo as a function of stellar mass according to the model presented in Sect. 2.1 for two metallicities. For comparison, we show measurements for the Milky Way (Gupta et al. 2017, using the stellar mass estimate of 6 × 1010 M⊙ from Bovy & Rix 2013 and Taylor et al. 2016) and the massive spiral galaxy NGC 6753 (Bogdán et al. 2017).
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