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ISM d ust model Monte Carlo dust radiative transfer

PAH in 3D. Shadows, gaps and ring-like structures in proto-planetary disks. Ralf Siebenmorgen, Frank Heymann , Nikolai Voshchinikov , Endrik Kr ű gel Peter Scicluna (PhD). ISM d ust model Monte Carlo dust radiative transfer Proto-planetary disks: ring-like structures

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ISM d ust model Monte Carlo dust radiative transfer