Spinning black holes magnetically connected to a Keplerian disk - Magnetosphere, reconnection sheet, particle acceleration, and coronal heating

Open Access

Fig. 12.

Map of synchrotron emission power for a BH spin a = 0.8, multiplied by r² to highlight the contribution from the current sheet. Photons emitted from the region delimited with with a dotted line are those shown as originating from the current sheet in the synthetic images in Figs. 13 and C.1.

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