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We report results on the spectroscopic follow-up of Nova SMC 2001 and NovaLMC 2002 carried out at La Silla. The analysis of the spectroscopic evolutionshows that these objects belong to the {\sl Fe II} class, according to theCerro Tololo scheme. From the line fluxes and the expansion velocities, we havederived an approximate mass for the ejected shells of 2$\div3\times 10^{-4}M_\odot$. The filling factor measurements ($\epsilon\sim 10^{-4}\div 10^{-1}$)suggest a clumpy structure for the ejecta.Comment: 11 pages+5 figures A&A in pres

Early decline spectra of nova SMC 2001 and nova LMC 2002