Abstract
In a 1st step I present results from our new set of evolutionary synthesis models for Simple (= single burst) Stellar Populations (SSPs) of various metallicities, and in a 2nd step I combine these results with the information we have about the redshift evolution of spiral galaxies’ ISM abundances. The aim is to provide a grid of color and luminosity distibutions of any secondary GC population formed at some time in the past in those mergers for comparison with observations.
| Original language | English |
|---|---|
| Title of host publication | In: Procs of Extragalactic Star Clusters - IAU Symposium 207 |
| Publisher | Astronomical Society of the Pacific |
| Pages | 642-8 |
| Publication status | Published - 2002 |
Fingerprint
Dive into the research topics of 'Predicting Metallicities and Color Distributions for Secondary GCs Forming in Spiral Galaxy Mergers at Various Redshifts'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver