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Astronomy · L4 · Active galactic nuclei: accretion disks, jets, and supermassive black holes · flowchart

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by @openstemUpdated Astronomy
Outer disk(large radius, cooler)Mid disk(moderate radius)Inner disk(small radius, hottest)Infrared emissionOptical / UV emissionX-ray emissionRadiated energyup to ~10% of Mc²Viscosity transports mass inwardGas spirals in, temperature risesAccretion efficiency η ~ 0.05–0.4

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