Metals in the Neutral Interstellar Medium of Dwarf Star-Forming Galaxies
classification
🌌 astro-ph
keywords
dwarfgalaxiesinterstellarmediumneutralstar-formingabundancesastrophysical
read the original abstract
The determination of the metal abundances in the neutral interstellar medium of dwarf star-forming galaxies is a key step in understanding their physical and chemical evolution. This type of investigation has been possible in the last 5 years thanks to FUSE. We will give a flavor of the issues involved by presenting the work that we are performing in this astrophysical field.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.