TY - JOUR
T1 - Chemical abundances of H II regions in the starburst galaxy NGC 1705
AU - Lee, Henry
AU - Skillman, Evan D.
PY - 2004/10/20
Y1 - 2004/10/20
N2 - We report optical spectroscopy of 16 H II regions in NGC 1705 and [O III] λW363 detections for the first time in five H II regions. The resulting mean oxygen abundance derived directly from measured electron temperatures is 12 + log(O/H) = 8.21 ± 0.05, which corresponds to [O/H] = -0.45, or 35% of the solar value. There are no significant spatial inhomogeneities in [O III] λ4363 oxygen abundances from H II regions at a radius approximately 10″ from the super star cluster. In H II regions where [O III] λ4363 was not measured, oxygen abundances derived with bright-line methods (accurate only to 0.2 dex) are in agreement with direct values of the oxygen abundance. Faint, narrow He II λ4686 emission is found in two H II regions, but the implied contribution from O+3 to the total oxygen abundance is only 0.01 dex. The mean argon-, neon-, and nitrogen-to-oxygen abundance ratios are consistent with mean values for other dwarf irregular galaxies, blue compact dwarf galaxies, and H II galaxies at comparable oxygen abundances. Interestingly, the nitrogen-to-oxygen abundance ratio in the ionized H II gas agrees with the value for the neutral H I, even though the metallicity of the neutral gas may be a factor of 6 lower than that of the ionized gas. This may be indicative of low-metallicity gas in the halo of the galaxy. Extinction values, Av, derived from observed Balmer line ratios along lines of sight to H II regions are in the range between 0 and 0.9 mag. Significant and variable extinction may have important effects on the interpretation of resolved stellar populations and derived star formation histories. With respect to the metallicity-luminosity and metallicitygas fraction diagnostics, the measured oxygen abundance for NGC 1705 is comparable to those of Local Group dwarf irregular galaxies at a given luminosity and gas fraction. Simple chemical evolution models suggest that the galaxy is quickly evolving into a gas-poor dwarf galaxy.
AB - We report optical spectroscopy of 16 H II regions in NGC 1705 and [O III] λW363 detections for the first time in five H II regions. The resulting mean oxygen abundance derived directly from measured electron temperatures is 12 + log(O/H) = 8.21 ± 0.05, which corresponds to [O/H] = -0.45, or 35% of the solar value. There are no significant spatial inhomogeneities in [O III] λ4363 oxygen abundances from H II regions at a radius approximately 10″ from the super star cluster. In H II regions where [O III] λ4363 was not measured, oxygen abundances derived with bright-line methods (accurate only to 0.2 dex) are in agreement with direct values of the oxygen abundance. Faint, narrow He II λ4686 emission is found in two H II regions, but the implied contribution from O+3 to the total oxygen abundance is only 0.01 dex. The mean argon-, neon-, and nitrogen-to-oxygen abundance ratios are consistent with mean values for other dwarf irregular galaxies, blue compact dwarf galaxies, and H II galaxies at comparable oxygen abundances. Interestingly, the nitrogen-to-oxygen abundance ratio in the ionized H II gas agrees with the value for the neutral H I, even though the metallicity of the neutral gas may be a factor of 6 lower than that of the ionized gas. This may be indicative of low-metallicity gas in the halo of the galaxy. Extinction values, Av, derived from observed Balmer line ratios along lines of sight to H II regions are in the range between 0 and 0.9 mag. Significant and variable extinction may have important effects on the interpretation of resolved stellar populations and derived star formation histories. With respect to the metallicity-luminosity and metallicitygas fraction diagnostics, the measured oxygen abundance for NGC 1705 is comparable to those of Local Group dwarf irregular galaxies at a given luminosity and gas fraction. Simple chemical evolution models suggest that the galaxy is quickly evolving into a gas-poor dwarf galaxy.
KW - Galaxies: abundances
KW - Galaxies: evolution
KW - Galaxies: individual (NGC 1705)
KW - Galaxies: irregular
KW - Galaxies: starburst
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U2 - 10.1086/423735
DO - 10.1086/423735
M3 - Article
AN - SCOPUS:10044248598
SN - 0004-637X
VL - 614
SP - 698
EP - 715
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2 I
ER -