Be-9 abundances in dwarfs of intermediate metal deficiency - Implications for galactic evolution
This paper presents observations of the 3130 A Be II resonance doublet in stars of intermediate metal deficiency, with Fe/H values between -0.6 and -1.1, obtained with the Intermediate Dispersion Spectrographs and IPCS detector at the 2.5 m Isaac Newton Telescope on La Palma. The derived beryllium abundances range from 5.6 x 10 to the -12th (one
Beckman, J. E. et al.
Fecha de publicación:
7
1989