We present preliminary results of 3-D hydro simulations of the interstellar medium evolution in dwarf spheroidal galaxies undergoing star formation for the first time. The star formation is assumed to occur in a sequence of instantaneus bursts separated by quiescent periods. Different models are made changing the number and the intensity of the bursts in such a way that the final mass of the formed stars remains the same. We followed the enrichment of the ISM taking into account the contribution of both type la and II supernovae. The aim of our models is to find a star formation history compatible with the observed spread of stellar age and metallicity in such galaxies and to reproduce the observed mass-metallicity relation. © 2005 International Astronomical Union.
Marcolini, A., Brighenti, F., D'Ercole, A. (2005). D Simulations of the ISM pollution by SNII and SNI in dwarf spheroidal galaxies. Cambridge University Press [10.1017/S1743921305003741].
D Simulations of the ISM pollution by SNII and SNI in dwarf spheroidal galaxies
MARCOLINI, ANDREA;BRIGHENTI, FABRIZIO;D'ERCOLE, ANNIBALE
2005
Abstract
We present preliminary results of 3-D hydro simulations of the interstellar medium evolution in dwarf spheroidal galaxies undergoing star formation for the first time. The star formation is assumed to occur in a sequence of instantaneus bursts separated by quiescent periods. Different models are made changing the number and the intensity of the bursts in such a way that the final mass of the formed stars remains the same. We followed the enrichment of the ISM taking into account the contribution of both type la and II supernovae. The aim of our models is to find a star formation history compatible with the observed spread of stellar age and metallicity in such galaxies and to reproduce the observed mass-metallicity relation. © 2005 International Astronomical Union.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
