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We adopt up-to-date yields of 7Li, 13C, 15N from classical novae and use awell tested model for the chemical evolution of the Milky Way in order topredict the temporal evolution of these elemental species in the solarneighborhood. In spite of major uncertainties due to our lack of knowledge ofmetallicity effects on the final products of explosive nucleosynthesis in novaoutbursts, we find a satisfactory agreement between theoretical predictions andobservations for 7Li and 13C. On the contrary, 15N turns out to be overproducedby about an order of magnitude.Comment: 8 pages, latex, 3 figures. To appear in "The Chemical Evolution of  the Milky Way: Stars versus Clusters", eds. F. Giovannelli and F. Matteucci  (Kluwer: Dordrecht

The Influence of Nova Nucleosynthesis on the Chemical Evolution of the Galaxy