Open Access

Fig. 6.

image

Download original image

Bolometric (upper panel) and X-ray (lower panel) luminosities vs. black hole mass of the sources considered in this work. Both luminosities scale with mass as M BH 0.6 $ M_{\mathrm{BH}}^{0.6} $, though the Lbol relation shows a larger correlation coefficient (r ∼ 0.7) than the LX relation (r ∼ 0.5).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.