Chemical abundances of Seyfert 2 AGNs - II. N2 metallicity calibration based on SDSS

被引:41
作者
Carvalho, S. P. [1 ]
Dors, O. L. [1 ]
Cardaci, M., V [2 ]
Hagele, G. F. [2 ]
Krabbe, A. C. [1 ]
Perez-Montero, E. [3 ]
Monteiro, A. F. [1 ]
Armah, M. [1 ]
Freitas-Lemes, P. [1 ]
机构
[1] Univ Vale Paraiba, UNIVAP, Av Shishima Hifumi 2911, BR-12244000 Sao Jose Dos Campos, SP, Brazil
[2] CONICET UNLP, Inst Astrofis La Plata, La Plata, Argentina
[3] CSIC, Inst Astrofis Andalucia, Camino Bajo de Huitor S-N,Aptdo 3004, E-18080 Granada, Spain
基金
巴西圣保罗研究基金会;
关键词
galaxies: abundances; galaxies: active; galaxies: evolution; galaxies: formation; galaxies: ISM; galaxies: nuclei; galaxies: Seyfert; EMISSION-LINE DIAGNOSTICS; ACTIVE GALACTIC NUCLEI; DIGITAL SKY SURVEY; OXYGEN ABUNDANCE; HII-REGIONS; NITROGEN ABUNDANCES; GAS METALLICITY; STAR-FORMATION; GALAXIES; EVOLUTION;
D O I
10.1093/mnras/staa193
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a semi-empirical calibration between the metallicity (Z) of Seyfert 2 active galactic nuclei and the N2 = log([N HP.6584/11 cy) emission-line intensity ratio. This calibration was derived through the [0 m]..5007/[0 u[),3727 versus N2 diagram containing observational data and photoionization model results obtained with the CLOUDY code. The observational sample consists of 463 confirmed Seyfert 2 nuclei (redshift z < 0.4) taken from the Sloan Digital Sky Survey DR7 data set. The obtained Z N2 relation is valid for the range 0.3 r< ( Z/Zo) 2.0 that corresponds to 0.7 < (N2) < 0.6. The effects of varying the ionization parameter (U), electron density and the slope of the spectral energy distribution on the Z estimations are of the order of the uncertainty produced by the error measurements of N2. This result indicates the large reliability of our Z N2 calibration. A relation between U and the IOutj/[OIII line ratio, almost independent of other nebular parameter, was obtained.
引用
收藏
页码:5675 / 5683
页数:9
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