New semianalytical intensity formulas and transfer functions cover static, infalling, and rotating thin accretion geometries on Schwarzschild black holes, working for all impact parameters.
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Black hole images under spherical-shell and circular-annulus accretion models in Schwarzschild spacetime: a semianalytical approach
New semianalytical intensity formulas and transfer functions cover static, infalling, and rotating thin accretion geometries on Schwarzschild black holes, working for all impact parameters.