Semi-empirical metallicity calibrations based on ultraviolet emission lines of type-2 AGNs
arXiv:1905.00691 · doi:10.1093/mnras/stz1242
Abstract
We derived two semi-empirical calibrations between the metallicity of the Narrow Line Region (NLR) of type-2 Active Galactic Nuclei and the rest-frame of the N V1240/He II, C43=log[(C IV+C III])/HeII] and C III]/C IV emission-line intensity ratios. A metallicity-independent calibration between the ionization parameter and the C III]/C IV emission-lines ratio was also derived. These calibrations were obtained comparing ratios of measured UV emission-line intensities, compiled from the literature, for a sample of 77 objects (redshift ) with those predicted by a grid of photoionization models built with the Cloudy code. Using the derived calibrations, it was possible to show that the metallicity estimations for NLRs are lower by a factor of about 2-3 than those for Broad Line Regions (BLRs). Besides we confirmed the recent result of the existence of a relation between the stellar mass of the host galaxy and its NLR metallicity. We also derived a relation for the objects in our sample at . This relation seems to follow the same trend as the ones estimated for Star Forming galaxies of similar high redshifts but for higher masses.
arXiv comment15 pages, MNRAS accepted
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