Fig. 11.
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Hβ (left panels), He I 5876 Å (middle panels) and N III 4100 Å (right panels) line luminosities as a function of RBB (upper panels) and TBB (lower panels). The dashed lines are the best fits for the data; linear for RBB and inverse power-law for TBB. The dotted-dashed line in the bottom panels is an inverse power-law fit with the exponent fixed at 2.
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