Abstract
We simulate the chemodynamical evolution of elliptical galaxies using our GRAPE-SPH code. We succeed in reproducing the observed variety of the radial metallicity gradients, from which we discuss the origin of elliptical galaxies.
| Original language | English |
|---|---|
| Pages (from-to) | 853-856 |
| Number of pages | 4 |
| Journal | Astrophysics and Space Science |
| Volume | 284 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - Apr 2003 |
Keywords
- EVOLUTION