We present the results of a series of simulations which study the influence of supernovae winds on the evolution of the baryonic component in Standard CDM models. In particular, our study has been focused on the evolution of the intercluster medium and on the L-T relation in galaxy clusters.
Hydrodynamical Simulations of X-ray Clusters with Supernova Heating
PANTANO, ORNELLA;
1999
Abstract
We present the results of a series of simulations which study the influence of supernovae winds on the evolution of the baryonic component in Standard CDM models. In particular, our study has been focused on the evolution of the intercluster medium and on the L-T relation in galaxy clusters.File in questo prodotto:
Non ci sono file associati a questo prodotto.
Pubblicazioni consigliate
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
