Highlight
Free Access

Fig. 11.

image

Download original image

Influence of the black hole spin, a, on the spectral and structural properties of our M 87 simulations. The left column corresponds to a MAD model, and the right column shows a SANE model. Top panels: broad-band spectrum averaged for 2000 M for thermal and five different spin values astar = −0.9375, −0.5, 0, 0.5, and 0.9375 (colour-coded) while keeping Rlow = 1, Rhigh = 160 σcut = 3.0, and ε = 0.5 fixed. The middle image shows the ray-traced 86 GHz images for different spin values. Bottom panels: jet diameter and opening angles profiles using the same colour-coding as for the spectrum.

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.