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 |
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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