Fluorine nucleosynthesis in low-mass AGB stars during the thermal pulse phase.

Details Fluorine nucleosynthesis in low-mass AGB stars during the thermal pulse phase. Fluorine nucleosynthesis in low-mass AGB stars during the thermal pulse phase.

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acaps..16...57l&link_type=abstract

Acta Astrophys. Sin., Vol. 16, No. 1, p. 57 - 64

Astronomy and Astrophysics

Astrophysics

Nucleosynthesis: Agb Stars, Nucleosynthesis: Low-Mass Stars

Scientific paper

19F production in low-mass AGB stars during the thermal pulse phase is studied, when the 13C-supply is introduced into the helium burning shell in a progressive way. The authors provide detailed calculations for the process with a parameterized model of H/He-burning. Compared with similar calculations when the 13C-supply is ingested instantaneously, they found that 19F can be synthesized too, but in a narrow T (temperature) range of 1.8 ≤ T/108K < 2.8. Comparisons between the computed correlations ([F/O], C/O), and that of observations are then presented.

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