Fig. 9
Fraction of the molecular DNM in the total H2
column-density (
)
derived fromthe dust (left) and γ-ray
(right) analyses for the anticentre (top) and Chamaeleon (bottom) regions. The DNM is assumed to be
50%
molecular. The white contours outline the shapes of the CO clouds at the
7 K km s−1
level chosen to separate DNM and COsat
components.
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