The relationship between the emission line, continuum luminosity, and Baldwin effect in blazars - I. The case of the Mg II λ2798 Å emission line

Open Access

Fig. 9.

BE for the 3000 Å continuum and the Mg II λ2798 Å emission line, using binned data, for disk-dominated (DD) sources (blue), jet-dominated (JD) sources (red), and objects with NTD < 1 (green). The left panel displays the BE for the RQ sources, while the right panel shows it for the FSRQ sources.

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