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Fig. 8


The “reddening” curve in the mid-IR, “normalized excess” = E(λ   −   Ks)/E(I − Ks) vs. wave number, for six stars behind the B 335 globule. The normalized excess derived from the Spitzer/ISOCAM spectra of two of the stars, #2 and # 947, are included with the same normalization.

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