The origin of fluorine: abundances in AGB carbon stars revisited

201570 citationsJournal Articlebronze Open Access

Authors

S. Cristallo · Istituto Nazionale di Fisica Nucleare, Sezione di Napoli

P. de Laverny · Observatoire de la Côte d’Azur

Abstract

Context. Revised spectroscopic parameters for the HF molecule and a new CN line list in the 2.3 μm region have recently become available, facilitating a revision of the F content in asymptotic giant branch (AGB) stars.

Topics & Keywords

Astrophysics and Star Formation Studies Stellar, planetary, and galactic studies Astro and Planetary Science

Publication Details

Published in: Astronomy and Astrophysics

Volume 581, pp. A88-A88

DOI: 10.1051/0004-6361/201526586

Field-Weighted Citation Impact: 3.75

Command Palette

The origin of fluorine: abundances in AGB carbon stars revisited

Authors

Abstract

Topics & Keywords

Publication Details