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MPIfR Optical & Infrared Interferometry Group


T. Driebe and T. Blöcker:

Stellar Evolution for Low and Intermediate-Mass Stars with Rotation and Overshoot

Abstract (poster) for:
Astronomische Gesellschaft Meeting Abstracts (AGM 15, P19) New Astrophysical Horizons
Annual Scientific Meeting of the Astronomische Gesellschaft, Sep 21-25, 1999, Göttingen, Germany


Abstract. We expanded our stellar evolution code to treat the effects of rotation on the structure and evolution of low and intermediate mass stars. For this purpose we included the centrifugal term in the hydrostatic equation, considered angular momentum transport and took into account rotation induced mixing processes as in Heger et al. (1999). Convective overshoot was considered according to the hydrodynamical simulations of Freytag et al. (1996) recently being introduced to AGB models by Herwig et al. (1997). Additionally we used a coupled scheme of nucleosynthesis and mixing.
In this exploratory study we investigate the effects of rotation and overshoot on low and intermediate-mass stars on the main sequence and beyond. The width of the main sequence depends on the extent of the convective core and therefore on the mixing processes considered. We focus on the question if in the case of rotation a certain amount of overshoot is still required to model the observed width of the main sequence. Abundance ratios as, for instance, C12/C13, constrain the efficiency of the various mixing treatments and are studied for different evolutionary stages.

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bloecker@speckle.mpifr-bonn.mpg.de.
Last modified on 20-Sep-99.
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