Fig. 11
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Foreground components in the ROSAT map with the eROSITA bubble contour overlaid. This foreground maps was built by Freyberg (1994), who modeled and separated the foreground emissions from RASS map. The resulting maps are shown with the angular resolution of 0.2°. We overlay the contour of eROSITA bubbles (defined from 0.6–1.0 keV band) as a white translucent area.
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