High carbon in I Zwicky 18: New results from hubble space telescope spectroscopy

D. R. Garnett, E. D. Skillman, R. J. Dufour, G. A. Shields

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Abstract

We present new measurements of the gas-phase C/O abundance ratio in both the northwest (NW) and southeast (SE) components of the extremely metal-poor dwarf irregular galaxy I Zw 18, based on ultraviolet spectroscopy of the two H II regions using the Faint Object Spectrograph on the Hubble Space Telescope. We determine values of log C/O = -0.63 ± 0.10 for the NW component and log C/O = -0.56 ± 0.09 for the SE component. In comparison, log C/O = -0.37 in the Sun, while log C/O = -0.85 ± 0.07 in the three most metal-poor irregular galaxies measured by Garnett et al. Our measurements show that C/O in I Zw 18 is significantly higher than in other comparably metal-poor irregular galaxies and above predictions for the expected C/O from massive star nucleosynthesis. These results suggest that carbon in I Zw 18 has been enhanced by an earlier population of lower-mass carbon-producing stars; this idea is supported by stellar photometry of I Zw 18 and its companion, which demonstrate that the current bursts of massive stars were not the first. Despite its very low metallicity, it is likely that I Zw 18 is not a "primeval" galaxy.

Original languageEnglish (US)
Pages (from-to)174-178
Number of pages5
JournalAstrophysical Journal
Volume481
Issue number1 PART I
DOIs
StatePublished - 1997

Keywords

  • Galaxies: ISM
  • Galaxies: abundances
  • Galaxies: evolution
  • Galaxies: individual: I Zw 18
  • Galaxies: irregular

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