Seyfert AGN — Accretion Disk Multi-Temperature Spectrum
10⁷·⁵ M☉
0.10 Ṁₑ
0.50
30°
1.80
0.10
Disk (multi-BB)
X-ray Corona
IR Torus
Total SED
Shakura-Sunyaev disk: T(r) ∝ (M·Ṁ)^(1/4) · r^(-3/4). Multi-color blackbody: each annulus emits as Planck function. ISCO depends on spin (r_ISCO = 1–9 Rg). X-ray corona: power-law Γ. IR from dusty torus reprocessing. SED spans radio to X-ray.