Revisiting the radial abundance gradients of nitrogen and oxygen of the Milky Way
C. Esteban, J. Garcia-Rojas

TL;DR
This study provides new insights into the radial abundance gradients of nitrogen and oxygen in the Milky Way's disc, revealing a nearly flat N/O ratio and potential flattening of oxygen abundance in the inner Galaxy, based on spectroscopic data of HII regions.
Contribution
It introduces a new, ionisation correction factor-independent measurement of nitrogen abundance gradients and reassesses oxygen gradients with a larger, homogeneous dataset.
Findings
Nitrogen abundance gradient is independent of ionisation correction factors.
The N/O ratio remains nearly flat across the Galactic disc.
Possible flattening or drop of oxygen abundance in the inner Galaxy.
Abstract
We present spectra obtained with the 10.4 m Gran Telescopio Canarias telescope of 13 Galactic HII regions, most of them of very low ionisation degree. The objects are located along the Galactic disc, with R_G from 5.7 to 16.1 kpc. We determine T_e([NII]) for all of them. We obtain - for the first time - a radial abundance gradient of N that is independent on the ionisation correction factor. The radial distribution of the N/O ratio is almost flat, indicating that the bulk of N is not formed by standard secondary processes. We have made a reassessment of the radial O abundance gradient combining our results with previous similar ones by Esteban et al. (2017); producing a homogeneous dataset of 35 HII regions with direct determinations of the electron temperature. We report the possible presence of a flattening or drop of the O abundance in the inner part of the Galactic disc. This result…
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