Combining [N II] electron temperatures with [O II] auroral-to-nebular densities yields HII-region oxygen abundances less biased by density inhomogeneities, with the abundance discrepancy factor possibly larger in metal-rich regions.
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Toward Unbiased Abundance Measurements in Inhomogeneous $\mathrm{H\,II}$ Regions
Combining [N II] electron temperatures with [O II] auroral-to-nebular densities yields HII-region oxygen abundances less biased by density inhomogeneities, with the abundance discrepancy factor possibly larger in metal-rich regions.