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(1 - 4 of 4)
Mapping the evolution of pure CO2 ices irradiated by ions, UV, and electrons using the upgraded PROCODA code (employing an effective rate constant ordering by thermochemistry data)
The impact of stochastic modelling on the predictive power of galaxy formation simulations
EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
Punctuated chaos and the unpredictability of the Galactic Centre S-star orbital evolution