Fig. 7
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Finding chart for features discussed mainly in Sect. 3.4 and 4.2. The background image shows the emission measure of the LHB, which is a proxy of the extent of the LHB and is relevant for discussions (Sect. 4.2) on interstellar tunnels and anti-correlation with dust. The demarcation of the eROSITA bubbles is shown by the turquoise line, based on the 0.6–1.0 keV intensity map.
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