GEOMETRY DEPENDENT. “If the geometry of absorbing and scattering material is known or assumed, then radiative transfer models can be used to predict the SED of a galaxy, which should differ depending on whether the source of heating is a very small AGN with a very hard UV SED, or a more extended, softer-spectrum nuclear star-forming region. Note that the results are expected to be very sensitive to the assumed geometry.” (AGN = active galactic nuclei; UV = ultraviolet; SED = spectral energy distributions).
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