Alexander Schäbe
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View article: HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations
HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations Open
Aims . We present a new sub-grid model, HYACINTH – HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations – for computing the non-equilibrium abundances of H 2 and its carbon-based tracers, namely CO, C, and C + , in…
View article: A comparison of H2 formation models at high redshift
A comparison of H2 formation models at high redshift Open
Modelling the molecular gas that is routinely detected through CO observations of high-redshift galaxies constitutes a major challenge for ab initio simulations of galaxy formation. We carry out a suite of cosmological hydrodynamic simulat…