Comparing rotation curve observations to hydrodynamic {\Lambda}CDM simulations of galaxies

Understand

The formation of the disk and feedback from supernova winds impacts the distribution of dark matter in galaxies.

• Recently, Di Cintio et al.
• (2014b) characterized the halo response from baryonic processes in hydrodynamical simulations via a dependence on the ratio of stellar-to-halo mass ($M_{\star}/M_{{\rm halo}}$).
• The (stellar) mass dependent halo profile links together the local and global properties of the halo (e.g.