Other
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..255..278l&link_type=abstract
Low-Metallicity Star Formation: From the First Stars to Dwarf Galaxies, Proceedings of the International Astronomical Union, IAU
Other
Ism: Abundances, (Ism:) Hii Regions, Galaxies: Abundances, Galaxies: Dwarf, Galaxies: Starburst, Galaxies: Ism, Ultraviolet: Ism, Ultraviolet: Galaxies
Scientific paper
We derive the chemical composition of the neutral gas in the blue compact dwarf (BCD) Pox 36 observed with FUSE. Metals (N, O, Ar, and Fe) are underabundant as compared to the ionized gas associated with H ii regions by a factor ~7. The neutral gas, although it is not pristine, is thus probably less chemically evolved than the ionized gas. This could be due to different dispersal and mixing timescales. Results are compared to those of other BCDs observed with FUSE. The metallicity of the neutral gas in BCDs seems to reach a lower threshold of ~1/50 Z&sun; for extremely-metal poor galaxies.
Kunth Daniel
Lebouteiller Vianney
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