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

Astronomy and Astrophysics – Astrophysics

Scientific paper

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4 pages, 3 figures, to appear in the proceedings of JENAM 2005, Liege 4-7 July 2005

Scientific paper

10.1553/cia147s89

In main-sequence stars, the chemical composition gradient that develops at
the edge of the convective core is responsible for a non-uniform period spacing
of high-order gravity modes. In this work we investigate, in the case of a 1.6
Msun star, the effects on the period-spacing of extra mixing processes in the
core (such as diffusion and overshooting).

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