Technetium and the third dredge up in AGB stars II. Bulge stars

@inproceedings{Uttenthaler2006TechnetiumAT,
  title={Technetium and the third dredge up in AGB stars II. Bulge stars},
  author={Stefan Uttenthaler and J. Hron and Thomas Lebzelter and Maurizio Busso and Mathias Schultheis and Hans Ulrich Kaeufl Eso Garching and Dept. of Physics Astronomy and University of Vienna and Austria and Dept. of Physics and Univ. of Perugia and Italy. and Observatoire de Besançon and France.},
  year={2006}
}
Context. We searched for Technetium (Tc) in a sample of bright oxygenrich asymptotic giant branch (AGB) stars located in the oute r galactic bulge. Tc is an unstable element synthesised via the s-proce ss in deep layers of AGB stars, thus it is a reliable indicator of both recent s-process activity and third dredge-up. Aims. We aim to test theoretical predictions on the luminosity lim it for the onset of third dredge-up. Methods. Using high resolution optical spectra obtained with the UVE S… 

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