New light on the search for low metallicity galaxies I. The N2 method

Abstract

We present a simple metallicity estimator based on the logarithmic [NII]6584 / Halpha ratio, hereafter N2, which we envisage will become very useful for ranking galaxies in a metallicity sequence from redshift survey quality data even for moderately low spectral resolution. We have calibrated the N2 estimator using a compilation of HII galaxies having accurate oxygen abundances, plus photoionization models covering a wide range of abundances. The comparison of models and observations indicates that both primary and secondary nitrogen are important for the relevant range of metallicities. The N2 estimator follows a linear relation with log(O/H) that holds for the whole abundance range covered by the sample, from about 1/50th to twice the Solar value (7.2 < 12+log(O/H) < 9.1). We suggest that the ([SII]6717,6731 / Halpha) ratio (hereafter S2) can also be used as a rough metallicity indicator. Because of its large scatter the S2 estimator will be useful only in systems with very low metallicity, where [NII]6584 is not detected or in low resolution spectra where [NII]6584 is blended with Halpha.