On the far-infrared metallicity diagnostics: applications to high-redshift galaxies
In an earlier paper we modelled the far-infrared emission from a star-forming galaxy using the photoionization code CLOUDY and presented metallicity sensitive diagnostics based on far-infrared fine structure line ratios. Here, we focus on the applicability of the [O III] 88 μm/[N II] 122 μm line ratio as a gas-phase metallicity indicator in high
Rigopoulou, D. et al.
Advertised on:
1
2018