Limit of the Convective Core in delta Scuti Stars

Details Limit of the Convective Core in delta Scuti Stars Limit of the Convective Core in delta Scuti Stars

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..349..281l&link_type=abstract

Astrophysics of Variable Stars, Pecs, Hungary, 5-10 September 2005, Sterken, C. and Aerts, C. (eds). ASP Conference Series, Vol.

Astronomy and Astrophysics

Astrophysics

Scientific paper

delta Scuti stars are variable stars pulsating in nonradial low-order p and g modes. The presence of a convective core during the main sequence influences the oscillation spectrum of such stars. We construct a grid of models covering a large panel of typical delta Scuti properties and we determine the most suitable oscillation mode to probe the deep stellar interior and to measure the extent of the convective core. We investigate the effect induced by different values of the overshooting parameter on the position of the limit of the convective core.

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