Analytic solutions and scaling laws for Lyman-alpha radiative transfer in homologously expanding clouds and hot cosmological flows are derived and validated with a gridless Monte Carlo method that tracks Doppler shifts continuously.
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Lyman-alpha resonant-line radiative transfer in expanding media
Analytic solutions and scaling laws for Lyman-alpha radiative transfer in homologously expanding clouds and hot cosmological flows are derived and validated with a gridless Monte Carlo method that tracks Doppler shifts continuously.