(see J.J. Cowan et al., Ap.J. 521 (1999) 194-205).
|
|
Elemental r-abundances calculated with ETFSI-Q masses (red line)
[J.M. Pearson et al., Phys. Lett. B387 (1996) 455] are
compared to the respective Nr,solar values (green filled circles).
Superimposed are measured abundances (blue filled squares) from the
metal-poor halo star CS22892-052 [C. Sneden et al., Ap. J. 591 (2003)
936], which were normalized to the solar rare-earth values (see J.J. Cowan et al., Ap.J. 521 (1999) 194-205). |