T7: Simulating a disk galaxy:
reproducing the SK relation

Before the tutorials:

As discussed in the Lecture, there is a famous relation observed in galaxies relating the surface density of gas with the star formation rate: the so-called SK relation.

During the tutorials:

You can start from several initial conditions of idealized galaxies:

Preparing the simulation:

Solutions

Example for analyzing the simulation

Extra

You can additionally switch on the kinetic feedback and see what happens, especially if now a galactic outflow/wind is established.

Useful commands