![Beyond the [OIII]4363 auroral line: [NeIII]3868 as a direct tracer of the electron temperature](/publication/2026-aa-710-l-28-p/featured_hu8295692603524777932.webp)
Beyond the [OIII]4363 auroral line: [NeIII]3868 as a direct tracer of the electron temperature
Alternative technique to derive physical properties in the photoionized ISM to extend both local and high-z studies.
Jun 19, 2026
From "The Cliff" to "Virgil": Mapping the Spectral Diversity of Little Red Dots with JWST/NIRSpec
May 20, 2026
Chemical enrichment in LINERs from MaNGA: II. Characterizing the shape of the radial metallicity gradients
The AGN feed(back) process alters the shape of radial metallicity gradients depending on how evolved the galaxy is, and which is the dominant source for gas kinematics.
Feb 18, 2026
Sulphur abundances in star-forming regions from optical emission lines: A new approach based on photoionization models consistent with the direct method
Jun 1, 2025
Exploring the hardness of the ionizing radiation with the infrared softness diagram: II. Bimodal distributions in both the ionizing continuum slope and the excitation in active galactic nuclei
Apr 1, 2025
Chemical enrichment in LINERs from MaNGA: I. Tracing the nuclear abundances of oxygen and nitrogen in LINERs with varied ionizing sources
Feb 1, 2025
Chemical abundances and deviations from the solar S/O ratio in the gas-phase interstellar medium of galaxies based on infrared emission lines
May 1, 2024
A departure from the mass-metallicity relation in merging galaxies due to an infall of metal-poor gas
Mergen-driven infall of metal-poor gas causes metallicity dillutation but enhances star formation, explaining observed properties of (U)LIRGs.
Mar 1, 2024
Assessing model-based carbon and oxygen abundance derivation from ultraviolet emission lines in AGNs
May 1, 2023
Measuring chemical abundances in AGN from infrared nebular lines: HII-CHI-MISTRY-IR for AGN
Oct 1, 2022