Chemical Evolution of the ISM in Nearby Galaxies
Abstract
Introduction and purpose Abundances from HII regions Simple chemical evolution Abundance patterns in dwarf galaxies Abundance patterns in spiral galaxies Self-consistent star formation histories Summary References
- Publication:
-
Stellar astrophysics for the local group: VIII Canary Islands Winter School of Astrophysics
- Pub Date:
- 1998
- Bibcode:
- 1998salg.conf..457S