Kavli Affiliate: Lina Necib | Summary:Ultra-faint dwarf galaxies (UFDs) in the Milky Way are ideal probes of low-mass galaxy formation and dark matter because they are highly dark-matter dominated. In the lowest-mass systems, however, unresolved binary orbital motion complicates dynamical mass estimates by inflating measured velocity dispersions and biasing the interpretation of the inferred masses. […]
Continue.. From observing strategies to velocity dispersion bias: forward modeling unresolved binaries in ultra-faint dwarf galaxies