Dense gas formation in the Musca filament due to the dissipation of a supersonic converging flow

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Fig. 5

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Histograms of the ¹²CO(4–3)/¹²CO(2–1) (blue) and ¹²CO(4–3)/¹²CO(3–2) (green) main beam brightness ratio for the pixels in the northern map with a ¹²CO(4–3) rms < 0.2 K. The dashed blue line indicates the average ¹²CO(4–3)/¹²CO(2–1) ratio for all pixels, and the dashed green line indicates the average ¹²CO(4–3)/¹²CO(3–2) ratio.

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