Fig. 7

Disk dust mass vs. effective temperature for a representative sample of intermediate-mass stars (see Garufi et al. 2018). Empty symbols indicate the presence of a disk cavity while the large and small horizontal bars indicate the presence of a known jet and micro-jet, respectively. Symbol sizes are proportional to the stellar mass with dynamic range from 1.5 to 3 M⊙ while the accretion rate is indicated by the color with strong accretors (>4 × 10−8 M⊙ yr−1) in red, medium accretors (down to 10−8 M⊙ yr−1) in orange, and low/no accretors in cyan. The dashed line separates TTSs and Herbig stars according to the formal threshold atF0 type.
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