Short-lived isotopes and 23Na production in low mass AGB Stars

Details Short-lived isotopes and 23Na production in low mass AGB Stars Short-lived isotopes and 23Na production in low mass AGB Stars

2006-06-15

arxiv.org/abs/astro-ph/0606374v1

Astronomy and Astrophysics

Astrophysics

6 pages, 3 figures; in the proceedings of the VIII Torino Workshop on Nucleosynthesis in AGB stars; to be published in Mem.SAI

Scientific paper

We discuss the synthesis of some short-lived isotopes and of 23Na in thermally pulsing AGB stars with initial mass of 2 Msun and two different metallicities (Z=1.5e-2, corresponding to the metal amount in the Sun, and Z=1e-4), representative of disk and halo stars, respectively. The different nucleosynthesis channels are illustrated in some details. As previously found, the 13C formed after each third dredge up episode is usually completely consumed by alpha captures before the onset of the subsequent thermal pulse, releasing neutrons. This is the most efficient neutron source in low mass AGB stars and the resulting s-process nucleosynthesis is at the origin of the solar main component. However, in the solar metallicity model, we find that the temperature of the first formed 13C pocket remains too low during the interpulse and the 13C is not completely burnt, being partially engulfed in the convective zone generated by the following thermal pulse. Due to the rapid convective mixing in this zone, the 13C is exposed to a larger temperature and a nucleosynthesis characterized by a relatively high neutron density develops. The main effect is the strong enhancement of isotopes located beyond some critical branching in the neutron-capture path, like 60Fe, otherwise only marginally produced during a standard s-process nucleosynthesis.

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