Fig. 11
Glass & Moorwood (1985) two color diagram. Moving away from the ordinary galaxy colors (black circle at J−H = 0.78 and H−K = 0.22) and along the horizontal lines in the loci of mixtures, there is an increasing percentage (10% per vertical line) of contribution from hot dust emission, while moving along the vertical lines, the temperature of this dust component increases (T ~ 500−1500 K).
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