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Fig. F.5

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Column density toward GMF41. These maps show the column densities of atomic hydrogen traced by H I emission, the cold hydrogen gas traced by HISA, and molecular hydrogen traced by 13CO emission, respectively. The column densities are integrated over the velocity range of the filament region given in Table 1. The white contours in both panels show the integrated MWISP 13CO emission at the levels 6.0, 12.0, 24.0, and 34.0 K km s−1. Left panel: H I column density traced by H I emission. Middle panel: HISA column density. Right panel: H2 column density traced by 13CO.

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