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The formation of CDM haloes II: collapse time and tides
Mikolaj Borzyszkowski, Aaron D. Ludlow, Cristiano Porciani
We use two cosmological simulations of structure formation in the LambdaCDM scenario to study the evolutionary histories of dark-matter haloes and to characterize the Lagrangian re…
Atomic carbon as a powerful tracer of molecular gas in the high-redshift Universe: perspectives for ALMA
Matteo Tomassetti, Cristiano Porciani, Emilio Romano-Diaz +2
We use a high-resolution hydrodynamic simulation that tracks the non-equilibrium abundance of molecular hydrogen within a massive high-redshift galaxy to produce mock Atacama Large…
Simulating the H2 content of high-redshift galaxies
Matteo Tomassetti, Cristiano Porciani, Emilio Romano-Diaz +1
We introduce a sub-grid model for the non-equilibrium abundance of molecular hydrogen in cosmological simulations of galaxy formation. We improve upon previous work by accounting f…