Fig. 5
Infrared slope as a function of mm flux. Millimeter fluxes are identical to F1300 or were converted from other wavelengths according to Eq. (1). Binaries are indicated with diamonds. For comparison, data from more massive T Tauri stars in the Chamaeleon star-forming region are shown (Cha I, Winston et al. 2012; Cha II, Spezzi et al. 2013).
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