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In main-sequence stars, the chemical composition gradient that develops atthe edge of the convective core is responsible for a non-uniform period spacingof high-order gravity modes. In this work we investigate, in the case of a 1.6Msun star, the effects on the period-spacing of extra mixing processes in thecore (such as diffusion and overshooting).Comment: 4 pages, 3 figures, to appear in the proceedings of JENAM 2005, Liege  4-7 July 200

Effects of "extra-mixing" processes on the periods of high-order gravity modes in main-sequence stars