Fig. 20

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Three-dimensional structure of the LHB in the western Galactic hemisphere assuming a constant density of 4 × 10−3 cm−3. The inner (opaque, coloured) and the outer (grey, translucent) surfaces show the ±1 σ uncertainty bounds of the distance under the constant ne assumption. We note that the two surfaces only reflect the uncertainty in the spectral fitting but not in ne. We note that kTLHB is also colour-coded on the inner surface. A sphere of 100 pc radius is shown around the Sun (yellow) as a ruler. An interactive version of this figure, including the comparison with dust maps (not shown) can be accessed from online or the accompanying website (Sect. 5).
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