We examine the relation between oxygen abundances in the narrow-line regions (NLRs) of active galactic nuclei (AGNs) estimated from the optical emission lines through the strong-line method (the theoretical calibration of Storchi-Bergmann et al. 1998), via the direct Te-method, and the central intersect abundances in the host galax- ies determined from the radial abundance gradients. We found that the Te-method underestimates the oxygen abundances by up to ∼2 dex (with average value of ~0.8 dex) compared to the abundances derived through the strong-line method. This con- firms the existence of the so-called ?temperature problem? in AGNs. We also found that the abundances in the centres of galaxies obtained from their spectra trough the stro...
For the first time, we establish a gas-phase abundance pattern calibration for quiescent galaxies us...
International audienceAims:Our aims are to estimate the validity of empirical methods, such as R23, ...
We investigate the discrepancy between oxygen abundance estimations for narrow-line regions of activ...
We examine the relation between oxygen abundances in the narrow-line regions (NLRs) of active galact...
We compare the oxygen abundance (O/H) of the narrow-line regions (NLRs) of Seyfert 2 AGNs obtained t...
For the first time, neon abundance has been derived in the narrow line region from a sample of Seyfe...
The compilation of published spectra of Galactic HII regions with available diagnostic [OIII]4363 li...
We determine the gas-phase oxygen abundance for a sample of 695 galaxies and H II regions with relia...
Using a large sample of 38,478 star-forming galaxies selected from the Second Data Release of the Sl...
We investigate the discrepancy between oxygen abundance estimations for narrow-line regions of activ...
For the first time, neon abundance has been derived in the narrow line region from a sample of Seyfe...
We compare the oxygen abundance (O/H) of the Narrow Line Regions (NLRs) of Seyfert 2 AGNs obtained t...
Chemical abundance determinations in Low-Ionization Nuclear Line Regions (LINERs) are especially com...
We investigate the discrepancy between oxygen abundance estimations for narrow-line regions of activ...
We investigate two chemical abundance calibrations for the narrow-line region (NLR) of active galaxi...
For the first time, we establish a gas-phase abundance pattern calibration for quiescent galaxies us...
International audienceAims:Our aims are to estimate the validity of empirical methods, such as R23, ...
We investigate the discrepancy between oxygen abundance estimations for narrow-line regions of activ...
We examine the relation between oxygen abundances in the narrow-line regions (NLRs) of active galact...
We compare the oxygen abundance (O/H) of the narrow-line regions (NLRs) of Seyfert 2 AGNs obtained t...
For the first time, neon abundance has been derived in the narrow line region from a sample of Seyfe...
The compilation of published spectra of Galactic HII regions with available diagnostic [OIII]4363 li...
We determine the gas-phase oxygen abundance for a sample of 695 galaxies and H II regions with relia...
Using a large sample of 38,478 star-forming galaxies selected from the Second Data Release of the Sl...
We investigate the discrepancy between oxygen abundance estimations for narrow-line regions of activ...
For the first time, neon abundance has been derived in the narrow line region from a sample of Seyfe...
We compare the oxygen abundance (O/H) of the Narrow Line Regions (NLRs) of Seyfert 2 AGNs obtained t...
Chemical abundance determinations in Low-Ionization Nuclear Line Regions (LINERs) are especially com...
We investigate the discrepancy between oxygen abundance estimations for narrow-line regions of activ...
We investigate two chemical abundance calibrations for the narrow-line region (NLR) of active galaxi...
For the first time, we establish a gas-phase abundance pattern calibration for quiescent galaxies us...
International audienceAims:Our aims are to estimate the validity of empirical methods, such as R23, ...
We investigate the discrepancy between oxygen abundance estimations for narrow-line regions of activ...