HIGHLIGHTS
- who: Astrophys Space Sci ( et al. from the (UNIVERSITY) have published the article: Stellar abundances of beryllium and CUBES, in the Journal: (JOURNAL)
- future: In the near future CUBES will likely be the only instrument offering the opportunity to measure Be abundances in samples of extremely metal-poor stars and in turn-off stars of globular clusters.
SUMMARY
Only the Be II 2 S-2 P0 resonance lines at ~3130 Å are now used to determine Be abundances in latetype stars. Some of these blending lines are still unidentified, as for example . . .
If you want to have access to all the content you need to log in!
Thanks :)
If you don't have an account, you can create one here.