Chemically Consistent Evolutionary Synthesis
arXiv:astro-ph/0210535 · doi:10.1023/A:1024014800146
Abstract
To account for the range of stellar metallicities in local galaxies and for the increasing importance of low metallicities at higher redshift we present chemically consistent models for the spectral and chemical evolution of galaxies over cosmological timescales. We discuss advantages, limitations and future prospects of our approach.
4 pages, klups.sty, klucite.sty To appear in {\sl The Evolution of Galaxies. III - From Simple Approaches to Self-consistent Models}, eds. G. Hensler, G. Stasinska, S. Harfst, P. Kroupa, Chr. Theis
References in corpus (10)
- The Rest Frame Optical Spectra of Lyman Break Galaxies: Star Formation, Extinction, Abundances, and Kinematics
- Spectroscopy of Outlying H II Regions in Spiral Galaxies: Abundances and Radial Gradients
- Keck Spectroscopy of Redshift z~3 Galaxies in the Hubble Deep Field
- Low-Metallicity Inhibition of Type Ia Supernovae and Galactic and Cosmic Chemical Evolution
- The Extreme Outer Regions of Disk Galaxies: I. Chemical Abundances of HII Regions
- Spectral & Photometric Evolution of Simple Stellar Populations at Various Metallicities
- The Abundances of Nitrogen and Oxygen in Damped Lyman Alpha Systems
- Galaxies at z=4 and the Formation of Population II
- Evidence for chemical evolution in the spectra of high redshift galaxies
- Chemically Consistent Evolutionary Models with Dust