ICM METALLICITY EVOLUTION: EFFECTS OF DYNAMICAL PROCESSES
We present a study on the origin of the metallicity evolution of the intracluster medium (ICM) by applying a semi-analytic model of galaxy formation to N-Body/SPH non-radiative cosmological simulations of clusters of galaxies. The results obtained for a set of clusters with virial masses of - 1:5 -...
Wedi'i Gadw mewn:
| Cyhoeddwyd yn: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Prif Awduron: | , , , |
| Fformat: | Artigo |
| Iaith: | Inglês |
| Cyhoeddwyd: |
Universidad Nacional Autónoma de México
2009
|
| Pynciau: | |
| Mynediad Ar-lein: | https://www.redalyc.org/articulo.oa?id=57115758077 |
| Tagiau: |
Dim Tagiau, Byddwch y cyntaf i dagio'r cofnod hwn!
|