Weak emission lines and chemical composition in ionized nebula
The analysis of emission line spectra of photoionized nebulae allows us to determine the chemical composition of the interstellar medium from the solar neighbourhood to the high-redshift star-forming galaxies. It stands as an essential tool for our knowledge of the nucleosynthesis and cosmic chemical evolution. The advent of the large aperture (10m
César
Esteban López
In force date
Not in force