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The Herschel view of circumstellar discs : a multiwavelength study of Chamaeleon I

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Figure

Figure 1. Distribution of different spectral types (Luhman 2007) for oursample.
Table 1. List of photometry sources and relevant wavelengths.
Figure 4. Spectral slope diagram of entire sample: ‘are FS sources, ‘+’ are Class Is, ‘□’◦’ are Class IIs and TDs, ‘∨’ are upper limits
Figure 6. Spectral slope diagram of entire sample: with symbols as inFig. 4.
+7

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