Decomposition of galactic X-ray emission with PHOX - Contributions from hot gas and X-ray binaries

Open Access

Fig. 8.

Same as Fig. 7, but for LMXB emission in the 0.5–8 keV band. The solid black line is the expected relation from the employed LMXB model in Eq. (1). The dashed black line is the same relation for a luminosity limit L_min of 5 × 10³⁷ erg s⁻¹. Data points (cyan triangles) are taken from Lehmer et al. (2020).

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