Fig. 2
Probability distribution functions for Gaussian components with selected Doppler temperatures
,
top: E(B−V)∕NHI
for latitudes |b| > 20°
(black) and for canonical thin H I (red dashed line) (Lenz et al. 2017) compared to distributions of partial
E(B− V)∕NHI
ratios at Doppler temperatures TD = 50, 100, 200, 400, and 800 K. Middle: E(B−V)∕(NHI + 2NH2) distributionsfor |b| > 20°. All components (black line) in comparison to scaled distribution at selected Doppler temperatures. Bottom:
E(B− V)∕(NHI + 2NH2) distributions now all-sky, but excluding CO–bright regions. The amplitudes of the partial distributions are scaled up by constant factors.
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