The Star Formation History of IZw18

The star formation history in IZw18 has been inferred from HST/WFPC2 archival data. This is done by comparing the derived V, B–V and V, V–I color-magnitude diagrams and luminosity functions with synthetic ones, based on various sets of stellar evolutionary tracks. At a distance of 10 Mpc, the stars resolved in the field of IZw18 allow for a lookback time up to 1 Gyr. We find that the main body is not experiencing its first episode of star formation. Instead, it has been forming stars over the last 0.5–1 Gyr, at a rate of ∼ 1–2× 10 M⊙yr kpc. A more intense activity of 6–16× 10 M⊙yr kpc has taken place between 15 and 20 Myr ago. For the secondary body, the lookback time is 0.2 Gyr at most and the uncertainty is much higher, due to the shallower diagrams and the small number of resolved stars. The derived range of star formation rate is 3–10× 10 M⊙yr kpc. The IMF providing the best fit to the observed stellar populations in the main body has a slope 1.5, much flatter than in any similar galaxy analyzed with the same method. In the secondary body, it is peaked at α ≃ 2.2, closer to Salpeter’s slope (α=2.35). Subject headings: galaxies: evolution — galaxies: individual (IZw18) — galaxies: irregular — galaxies: photometry — galaxies: stellar content