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This document presents a study on the distribution of cosmic ray electrons in star-forming galaxies, deriving explicit algebraic expressions for their steady-state number density based on diffusion equations. The authors emphasize the importance of these solutions for interpreting radio astronomical observations and understanding galaxy formation. The study also discusses the role of supernovae as a primary source of cosmic rays and the implications of energy losses on the propagation of relativistic electr

Author

sobigsothick

Language

EN