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

Open Access

Fig. 15

Distance at which the integration of N_H reaches 10²⁰ cm⁻² in the Lallement et al. (2022) (left) and Edenhofer et al. (2024) (right) dust cubes, as proxies of the extent of the local bubble. The empty regions in the map indicate that the integration does not reach N_H ≥ 10²⁰ cm⁻² before 400 pc.

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