Speaker
Cinthia Ragone Figueroa
(Instituto de Astronomía Teórica y Experimental (IATE) CONICET-UNC)
Description
In the metal-enriched interstellar medium, the abundance of molecular gas is primarily governed by the formation of H2 on dust grains, as well as its self-shielding and shielding by dust against photo-dissociation by the interstellar radiation field. The upcoming presentation intends to describe a sub-resolution model for forming molecular hydrogen in hydrodynamic simulation with dust description and encouraging results in predicting the properties of galaxies in cosmological boxes.
Primary author
Cinthia Ragone Figueroa
(Instituto de Astronomía Teórica y Experimental (IATE) CONICET-UNC)
