A self-consistent model of cosmic ray transport in molecular clouds with ballistic, diffusive, and hybrid scenarios applied to Taurus shows enhanced scattering on clump scales, suppressed diffusion coefficients, and elevated ionization rates.
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An updated Nautilus code reproduces experimental steady-state [H2O2]/[H2O] and [O3]/[O2] abundance ratios in proton-irradiated ices via chemical parameter tuning, but underpredicts the fluence needed and overestimates H2O loss.
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Multiwavelength Probes of Cosmic Ray Transport in Molecular Cloud Structures
A self-consistent model of cosmic ray transport in molecular clouds with ballistic, diffusive, and hybrid scenarios applied to Taurus shows enhanced scattering on clump scales, suppressed diffusion coefficients, and elevated ionization rates.
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Simulation of proton radiolysis of H2O and O2 ices with the Nautilus code
An updated Nautilus code reproduces experimental steady-state [H2O2]/[H2O] and [O3]/[O2] abundance ratios in proton-irradiated ices via chemical parameter tuning, but underpredicts the fluence needed and overestimates H2O loss.