We use high-resolution Hubble Space Telescope imaging observations of the young (∼ 15 − 25 Myr) star cluster NGC 1818 in the Large Magellanic Cloud to derive an estimate for the binary fraction of F stars (1.3 < M⋆/M⊙ < 1.6). This study provides the strongest constraints yet on the binary fraction in a young star cluster in a low-metallicity environment ([Fe/H] ∼ −0.4). Employing artificial sta...
