2023
DOI: 10.48550/arxiv.2302.12876
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Chemical abundances in Seyfert galaxies X. Sulphur abundance estimates

Abstract: For the first time, the sulphur abundance relative to hydrogen (S/H) in the Narrow Line Regions of a sample of Seyfert 2 nuclei (Sy 2s) has been derived via direct estimation of the electron temperature. Narrow emission line intensities from the SDSS DR17 [in the wavelength range 3000 < 𝜆(Å) < 9100] and from the literature for a sample of 45 nearby (𝑧 < 0.08) Sy 2s were considered. Our direct estimates indicate that Sy 2s have similar temperatures in the gas region where most of the S + ions are located in c… Show more

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