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Fig. 12
2D density distribution functions in the velocity range − 8 < vLSR < 8 km s−1 for CNM (left), LNM (middle), and WNM (right), showing the relations between phase fractions and column densities lg (NH ∕[cm−2]) for each phase. Top panel: positions with |b| > 20°, bottom panel: all sky data.
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