A STELLAR ENDGAME - THE BORN-AGAIN SAKURAI OBJECT

Citation
M. Asplund et al., A STELLAR ENDGAME - THE BORN-AGAIN SAKURAI OBJECT, Astronomy and astrophysics, 321(2), 1997, pp. 17-20
Citations number
21
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
00046361
Volume
321
Issue
2
Year of publication
1997
Pages
17 - 20
Database
ISI
SICI code
0004-6361(1997)321:2<17:ASE-TB>2.0.ZU;2-D
Abstract
The surface chemical composition of this remarkable star shows that it is hydrogen-deficient, carbon-rich and enriched in the light s-proces s elements. Spectra taken in May and October 1996 indicate a decrease in the surface hydrogen abundance by 0.7 dex in five months along with an increase in the abundances of Li, Sr, Y and Zr. The abundance chan ges are in agreement with the hypothesis of the star being a rapidly e volving ''born-again'' AGB star experiencing a final He-shell flash, s imilar to FG Sge. The C-12/C-13 ratio in October is very low, also sug gesting hydrogen ingestion. By chemical composi tion, Sakurai's object resembles the R Coronae Borealis (R CrB) stars.