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Fig. 2.

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Gas-to-dust ratio of the MCS in units of the Milky Way’s median value of N H E ( B V ) = ( 0.63 ± 0.05 ) × 10 22 cm 2 mag $ \frac{N_{\mathrm{H}}}{E\mathrm{(B-V)}}=(0.63\pm0.05)\times 10^{22}\frac{\mathrm{cm}^{-2}}{\mathrm{mag}} $. Contour lines mark the values that are between two and five times higher, for comparision with Welty et al. (2012) and Koornneef (1982). The circles mark the H I absorption lines detected by Kobulnicky & Dickey (1999, black), while the white one marks the MALS pointing position reported here.

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