Oxygen abundances in the most oxygen-rich spiral galaxies
arXiv:astro-ph/0601122 · doi:10.1111/j.1365-2966.2006.10033.x
Abstract
Oxygen abundances in the spiral galaxies expected to be richest in oxygen are estimated. The new abundance determinations are based on the recently discovered ff-relation between auroral and nebular oxygen line fluxes in HII regions. We find that the maximum gas-phase oxygen abundance in the central regions of spiral galaxies is 12+log(O/H)~8.75. This value is significantly lower than the previously accepted value. The central oxygen abundance in the Milky Way is similar to that in other large spirals.
arXiv comment8 pages, 7 postscript figures, accepted for publication in MNRAS
References in corpus (16)
- Spectroscopy of Outlying H II Regions in Spiral Galaxies: Abundances and Radial Gradients
- The Definitive Abundance of Interstellar Oxygen
- The Metallicity-Luminosity Relation, Effective Yields, and Metal Loss in Spiral and Irregular Galaxies
- Oxygen and nitrogen abundances in nearby galaxies. Correlations between oxygen abundance and macroscopic properties
- On the oxygen abundance determination in HII regions: High - metallicity regions
- Abundances of metal-rich H II regions in M51
- Galactic Metallicity Gradients Derived from a Sample of OB Stars
- Biases in abundance derivations for metal-rich nebulae
- A VLT study of metal-rich extragalactic H II regions. I. Observations and empirical abundances
- Carbon and Oxygen Galactic Gradients: Observational Values from HII Region Recombination Lines
- The Homogeneity of Interstellar Oxygen in the Galactic Disk
- Abundance determinations in HII regions: model fitting versus Te-method
- The oxygen abundance distribution in M101
- On the oxygen abundance in our Galaxy
- O/H in the Local Bubble
- On the relationship between auroral and nebular oxygen line intensities in spectra of HII regions
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