Fluorine production in thermal pulses on the asymptotic giant branch

Details Fluorine production in thermal pulses on the asymptotic giant branch Fluorine production in thermal pulses on the asymptotic giant branch

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...261..157f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 261, no. 1, p. 157-163.

Astronomy and Astrophysics

Astrophysics

62

Asymptotic Giant Branch Stars, Fluorine, Nuclear Astrophysics, Stellar Oscillations, Abundance, Stellar Composition, Stellar Evolution, Stellar Models

Scientific paper

A one-dimensional hydrodynamic stellar evolution code that includes a self-consistent treatment of the concomitant nucleosynthesis is used to compute the evolution of a 3-solar mass star from the T Tauri stage up to the asymtotic giant branch (AGB) phase, and the mechanisms of fluorine production that have been encountered during thermal pulses on the AGB are examined. The paper presents the first F abundance predictions for an AGB star of 3 solar masses and metallicity Z = 0.03.

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