Abundance differences between the neutral and the ionized gas of the dwarf galaxy IZw 36

Abundance differences between the neutral and the ionized gas of the dwarf galaxy IZw 36 Abstract. We present a FUSE spectroscopic study of the nearby gas–rich, metal–deficient blue compact dwarf (BCD) galaxy IZw 36. Atomic hydrogen and many metal lines are observed in absorption against the stellar continuum of young, massive stars embedded in the ionized region. Profile fitting of absorption lines allowed us to determine abundances and investigate the chemical composition of the neutral gas. This study present strong evidences that nitrogen is 16 +7 −8 times less abundant in the neutral gas with respect to the ionized gas (all uncertainties are 2σ). Similarly, the oxygen abundance estimated using phosphorus as a tracer is lower in the neutral gas by a factor 8 +17 −5. We also find that argon is underabundant by a factor 32 +8 −7 and that log (Ar i/O i)<−3.0 which is inconsistent with the solar value −2.1±0.1 (Lodders 2003), implying that argon is likely ionized into Ar ii in the neutral medium.