The SRG/eROSITA diffuse soft X-ray background - I. The local hot bubble in the western Galactic hemisphere

Open Access

Fig. 5

Scatter plot of $σ_{\log N_{H}}$ ${\sigma _{\log {N_{\rm{H}}}}}$ against solid angle of contour bins. A positive correlation between $σ_{\log N_{H}}$ ${\sigma _{\log {N_{\rm{H}}}}}$ and the contour bin area can be seen, as larger bins tend to capture a larger spread in N_H. The points are coloured according to their Galactic longitudes.

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