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Fig. 18

image

All sky 2D distribution functions, showing how frequent phase fractions of different phases are related to each other for |b| > 20° in the velocity range − 8 < vLSR < 8 km s−1. Top for CNM and LNM and bottom for CNM and WNM. Left panel: unconstrained H I data; right panel: filamentary H I structures only.

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