A fully analytic accretion model combining a thick disk, Gaussian ring bumps, and localized Gaussian spots is applied to Kerr ray tracing, generating images with multiple bright spots and arcs.
Ichimaru,Bimodal behavior of accretion disks: theory and application to Cygnus X-1 transitions.,Astrophys
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Construction of an analytic multi-component accretion environment and its application to Kerr black hole imaging
A fully analytic accretion model combining a thick disk, Gaussian ring bumps, and localized Gaussian spots is applied to Kerr ray tracing, generating images with multiple bright spots and arcs.