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We provide and describe a library of diffuse stellar radiation fields inspiral galaxies derived using calculations of the transfer of stellar radiationfrom the main morphological components - disks, thin disks, and bulges -through the dusty interstellar medium. These radiation fields areself-consistent with the solutions for the integrated panchromatic spectralenergy distributions (SEDs) previously presented using the same model. Becauseof this, observables calculated from the radiation fields, such as gamma-ray orradio emission, can be self-consistently combined with the solutions for theultraviolet/optical/submillimeter SEDs, thus expanding the range ofapplicability of the radiation transfer model to a broader range of wavelengthsand physical quantities. We also give analytic solutions for radiation fieldsin optically thin stellar disks, in stellar disks with one dust disk and instellar disks with two dust disks. The analytic solutions for the direct lightare exact and can be used as benchmarks. The analytic solutions with scatteringare only approximate, becoming exact only in the extreme optically thick limit.We find strongly contrasting solutions for the spatial distribution of theradiation fields for disks, thin disks and bulges. For bulges we find a strongdependence of the radiation fields on Sersic index.

Radiation fields in star-forming galaxies: the disk, thin disk and bulge