Dynamical friction in ultra-faint galaxies removes central dark matter via star-DM interactions, forming cores and compact stellar clusters with binaries.
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The Milky Way stellar halo follows a double power-law density profile with inner slope -3.3, outer slope -4.8, and break radius 17.4 kpc.
citing papers explorer
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Collisional Dynamics of Stars and Dark Matter in Ultra-Faint Galaxies
Dynamical friction in ultra-faint galaxies removes central dark matter via star-DM interactions, forming cores and compact stellar clusters with binaries.
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The Milky Way Tomography with Subaru Hyper Suprime-Cam. II. Global halo structure
The Milky Way stellar halo follows a double power-law density profile with inner slope -3.3, outer slope -4.8, and break radius 17.4 kpc.