Production and transfer of UV photons in non-homogeneous spherical clouds.

Computer Science

Scientific paper

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Interstellar Clouds: Uv Radiation, Interstellar Clouds: Cosmic Rays

Scientific paper

The authors computed the cosmic ray-induced UV flux in a homogeneous
spherical cloud as a function of the extinction and scattering
properties of dust. In the present work they extended the analysis to
the case of clouds with radial gas and dust density gradients.

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