S-process nucleosynthesis during Hot dredge-ups

✍ Scribed by L. Siess; S. Goriely

• Book ID: 103865917
• Publisher: Elsevier Science
• Year: 2005
• Tongue: English
• Weight: 252 KB
• Volume: 758
• Category: Article
• ISSN: 0375-9474
• DOI: 10.1016/j.nuclphysa.2005.05.104

✦ Synopsis

We present new results of the nucleosynthesis of s-elements in hot AGB stars. In the framework of the overshoot model, we show that the s-process nucleosynthesis depends sensitively on the thermodynamical conditions of the mixing zone and depending on the stellar mass and unknown overshoot parameter a large variety of s-process efficiencies can be found. We also provide a qualitative description of the production of s elements as a function of the stellar mass and metallicity. This mechanism could account for the large range of s-process efficiencies determined through the [Pb/Ce] values in low-metallicity stars.