A tight N/O–potential relation in star-forming galaxies.

We report a significantly tighter trend between gaseous N/O and |$M_*/R_\mathrm{ e}$| (a proxy for gravitational potential) than has previously been reported between gaseous metallicity and |$M_*/R_\mathrm{ e}$|⁠ , for star-forming galaxies in the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey. We argue this result to be a consequence of deeper potential wells conferring greater resistance to metal outflows while also being associated with earlier star-formation histories, combined with N/O being comparatively unaffected by metal-poor inflows. The potential–N/O relation thus appears to be both more resistant to short time-scale baryonic processes and also more reflective of a galaxy's chemical evolution state, when compared to previously considered relations. [ABSTRACT FROM AUTHOR]