Fluorine in red giant stars - Evidence for nucleosynthesis

Details Fluorine in red giant stars - Evidence for nucleosynthesis Fluorine in red giant stars - Evidence for nucleosynthesis

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...261..164j&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 261, no. 1, p. 164-187.

Astronomy and Astrophysics

Astrophysics

143

Abundance, Fluorine, Nuclear Astrophysics, Red Giant Stars, Astronomical Spectroscopy, Nuclear Fusion, Stellar Evolution

Scientific paper

Flourine abundances were determined in several K giants and asymptotic giant branch (AGB) stars, using the infrared vibration-rotation lines of HF. The data presented constitute the only available information on the fluorine abundance outside the solar system and provide invaluable clues to the question of the nucleosynthetic origin of F. The observations confirm that F production occurs at a He-burning site and constrain the current models of AGB stars.

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