Jessica May Hislop

• Build a full picture of star cluster formation and destruction in isolated dwarf galaxy simulations at solar mass resolution.
• Explore the effect of different star formation prescriptions as well as the inclusion of intermediate mass black holes on the populations of star clusters and nuclear star cluster formation.

Roles at MPA:

• Student representative
• Member of the MPA Corona Task Force

Computational astrophysics, Hydrodynamical simulations, Black holes, Dwarf galaxies.

Supervisor: Thorsten Naab/Volker Springel