par D'Orazi, Valentina;Lucatello, Sara;Lugaro, Maria;Gratton, Raffaele R.G.;Angelou, George;Bragaglia, Angela;Carretta, Eugenio;Alves-Brito, Alan;Ivans, Inese I.I.;Masseron, Thomas 
;Mucciarelli, Alessio
Référence Memorie della Societa Astronomica Italiana, Supplementi - Journal of the Italian Astronomical Society, Supplement, 84, 1, page (34-37)
Publication Publié, 2013
;Mucciarelli, AlessioRéférence Memorie della Societa Astronomica Italiana, Supplementi - Journal of the Italian Astronomical Society, Supplement, 84, 1, page (34-37)
Publication Publié, 2013
Article révisé par les pairs
| Résumé : | The light-element variations among globular cluster (GC) stars are nowadays accepted as the signature of self-enrichment from previous generations of stars. It is expected that these extinct progenitors experienced hot H-burning and, as fluorine is involved in the complete CNO cycle, the F abundance in GCs can provide new clues about the previous generation(s). Along with Na-O and Mg-Al anti-correlations, theory predicts an anti-correlation between F and Na and a positive correlation between F and O. Moreover, relatively low-mass AGB stars are F producers (and are also responsible for C+N+O and s-process element variations). We present our results on F abundances in four GCs (NGC 6656, NGC 6752, 47 Tucanae and ω Centauri), which exhibit notably different s-process and/or C+N+O abundance patterns. |
