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We investigate the three-dimensional structure of the nearby edge-on spiralgalaxy NGC 891 using 3D Monte Carlo radiative transfer models, with realisticspiral structure and fractally clumped dust. Using the spiral and clumpinessparameters found from recently completed scattered light models we producelower resolution SED models which reproduce the global UV-to-FIR SED of NGC891. Our models contain a color gradient across the major axis of the galaxy -similar to what is seen in images of the NGC 891. With minor adjustment our SEDmodels are able to match the majority of M51's SED, a similar galaxy at a nearface-on different inclination.

The 3-Dimensional Structure of NGC 891 and M51