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NIHAO-GIZMO: A Comparison of Simulated Disc Galaxies from GASOLINE and GIZMO

Speaker: Houzun Chen

Different feedback model

Fig1

Resolution is the key.

Different kinds of simulations

Fig2

Cooling, metal, and star formation

Fig3

The origin of cold gas

Fig4

Summary

Fig5

Q&A

How to control IMF?

Supernovae rate IMF. The evolution of the IMF has not been implemented.

Released under the MIT License.