Abundances of Be-9 in a sample of highly metal-deficient dwarfs - Implications for early galactic nucleosynthesis and primordial lithium
We have observed six highly metal-deficient dwarfs in the spectral range containing the resonance doublet of 9Be II at 3130 Å. Using the method of spectral synthesis we have evaluated the abundance of 9Be in these objects. In three of the stars, those with metallicities [Fe/H] -1.5 we set upper limits to the 9Be abundance, 9Be/H, below 2.5 10-12
Rebolo, R. et al.
Fecha de publicación:
3
1988