Loose threads: Parsec-scale filamentation in the high-Galactic-latitude molecular clouds MBM 3 and MBM 16

Open Access

Fig. 17

Ratio of 60 µm and 100 µm emission from IRIS survey for MBM 3 (left panel) and MBM 16 (right panel), that is a measure of dust temperature. The overplotted ¹²CO (1-0) contours span between 3 and 12 K km s^-1 in steps of 3 K km s^-1 for MBM 3 and 1.5, 3, 4.5 K km s^-1 for MBM 16. The color bar is the same for both maps.

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