Fig. 12
Mass accretion rate vs. stellar mass for objects in the η Cha cluster (red filled triangles; this work), the Lupus (black empty circles; Alcalá et al. 2017), and Chamaeleon I star forming regions (blue empty squares; Manara et al. 2016). RECX 5 and RECX 9 overlap in this presentation as they differ only slightly in stellar mass and mass accretion rate. Typical errors are indicated in the lower right corner.
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