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Fig. 6
FWHM of the Hβ line as a function of the Ṁacc of the objects. The blue points indicate the narrow symmetric line sources (NS) while multi-peaked line objects (MP) are flagged with a red point. Accretion rates of the sub-luminous objects have been corrected for their obscuration factor (see Alcalá et al. 2014, and Table 1).
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