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Fig. 24


Density estimates (solid black line) from spinning dust models that follow the observed trend between the AME emissivity j28 and G0. We also show the influence of AME emissivities half (j0 = 1.5 × 10-24 MJy sr-1 cm2 per H atom; triple-dot-dashed line) and twice as large (j0 = 6 × 10-24 MJy sr-1 cm2 per H atom; dashed line).

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