activity
20142023
most citedMetallicity evolution of AGNs from UV emission-lines based on a new index

68 citations · 220 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA202314 cited

Chemical abundances in Seyfert galaxies X. Sulphur abundance estimates

O. L. Dors, M. Valerdi, R. A. Riffel +12

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 th…

astro-ph.GA202319 cited

Oxygen abundances in the narrow line regions of Seyfert galaxies and the metallicity-luminosity relation

Mark Armah, Rogério Riffel, O. L. Dors +7

We present oxygen abundances relative to hydrogen (O/H) in the narrow line regions (NLRs) gas phases of Seyferts 1 (Sy 1s) and Seyferts 2 (Sy 2s) Active Galactic Nuclei (AGNs). We…

astro-ph.GA202212 cited

Chemical abundance of LINER galaxies -- Metallicity calibrations based on SDSS-IV MaNGA

C. B. Oliveira, A. C. Krabbe, J. A. Hernandez-Jimenez +5

The ionizing source of Low Ionization Nuclear Emission Regions (LINERs) is uncertain. Because of this, an empirical relation to determine the chemical abundances of these objects h…

astro-ph.GA201712 cited

Interaction effects on galaxy pairs with GeminiGMOS-III: Stellar population synthesis

A. C. Krabbe, D. A. Rosa, M. G. Pastoriza +4

We present an observational study of the impacts of the interactions on the stellar population in a sample of galaxy pairs. Long-slit spectra in the wavelength range 3440-7300 Å ob…

astro-ph.GA201740 cited

New metallicity calibration for Seyfert 2 galaxies based on the N2O2 index

C. S. Castro, O. L. Dors, M. V. Cardaci +1

We derive a new relation between the metallicity of Seyfert 2 Active Galactic Nuclei (AGNs) and the intensity of the narrow emission-lines ratio =log([N II]6584/[O II]3…

astro-ph.GA201616 cited

Effective temperature of ionizing stars of extragalactic HII regions

O. L. Dors, G. F. Hagelle, M. V. Cardaci +1

The effective temperature (Teff) of the radiation field of the ionizing star(s) of a large sample of extragalactic HII regions was estimated using the R= log([OII](3727)/[OIII]5007…