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

Open Access

Fig. 4.

SpT histogram of sources with accretion measurement in the literature (dashed lines, see Sect. 3.6) and the new data (solid lines) in Cha-I (left panel), Upper Scorpius (middle panel), and Ophiuchus (right panel). Each region follows the same color-coding as in Fig. 1.

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