Modelling the spectral energy distribution of galaxies III. Attenuation of stellar light in spiral galaxies
We present new calculations of the attenuation of stellar light from spiral galaxies using geometries for stars and dust which can reproduce the entire spectral energy distribution from the ultraviolet (UV) to the Far-infrared (FIR)/submillimeter (submm)
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
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