Evolution of the relation between the mass accretion rate and the stellar and disk mass from brown dwarfs to stars

Open Access

Fig. 12.

CDF of the accretion depletion timescale (Ṁ_acc/M_disk) of Ophiuchus (top panel), Lupus (middle), and Cha-I (bottom). The black lines represent the CDF of BDs and the colored lines that of stars with M_disk < 10⁻³ M_⊙ (color-coded by region as in Fig. 5). The dashed lines represent the same CDF excluding the upper limit measurements.

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