Fig. 2
Distribution of radiative moments-energy density R0 (long dashedblue line), flux R1 (solid black line) and pressure R2 (dashed red line) with r above an accretion disc with ṁ = 10. Radiative moments produced by various components of the disc, for example, (a) from corona RnC; (b) from outer disc RnD and (c) total radiative moments Rn.
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