Fig. 3
F100 and F160 as a function of mm fluxes. Millimeter fluxes are identical to F1300 or were converted from other wavelengths according to Eq. (1). To compare, T Tauri stars in Chamaeleon I and II are shown as plus and cross symbols in the bottom panel (Winston et al. 2012; Spezzi et al. 2013). The dotted lines show linear fits to all points except upper limits and binaries.
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