What Can We Learn from the Nitrogen Abundance of High-z Galaxies?

March 2025 • 2025ApJ...981..136S

Authors • Stiavelli, Massimo • Morishita, Takahiro • Chiaberge, Marco • Leethochawalit, Nicha • Norman, Colin • Ricotti, Massimo • Roberts-Borsani, Guido • Treu, Tommaso • Vanzella, Eros • Wyse, Rosemary F. G. • Zhang, Yechi • Boyett, Kit

Abstract • We present measurements of the gas-phase oxygen and nitrogen abundances obtained by applying the direct method to JWST NIRspec R ∼ 1000 spectroscopy for six galaxies at redshift greater than 3. Our measurements are based on rest-frame optical nitrogen [N II]_{λλ6548,6583} lines and are complemented by six additional objects from the literature at 3 ≤ z ≤ 6. We find that 9 out of 12 objects have values of log(N/O) that are compatible with those found for low-redshift, metal-poor, dwarf galaxies and for H II regions of more luminous local galaxies. However, 3 out of 12 objects have log(N/O) values that are overabundant compared to what is expected on the basis of their oxygen abundance. We explore a few standard scenarios to explain the observations and conclude that, within the limited statistics available to us, none of them can be definitely excluded even though we prefer dilution by pristine gas infall in between star formation bursts, as this is predicted by simulations to take place as a natural part of bursty star formation.

Links

• PDF https://iopscience.iop.org/article/10.3847/1538-4357/adb5f3/pdf
• ELECTR https://iopscience.iop.org/article/10.3847/1538-4357/adb5f3
• PREPRINT http://arxiv.org/abs/2412.06517