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This article has an erratum: [https://doi.org/10.1051/0004-6361/202348748e]


Fig. 3

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Ratio between the accretion and stellar luminosities vs. effective temperature. σ-Orionis sources are indicated by orange circles while stars in other young SFRs by gray symbols. The dotted and dashed lines represent the locus of the chromospheric emission defined by Manara et al. (2013b, 2017a). Downward triangles indicate the non-accretors identified in this work.

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