Fig. 8
Abundance pattern of CS 22892−052, CS 31082−001, HE 1332−0309 and HE 0105−6141, compared with the solar r-process pattern (solid line) scaled to the Eu abundance and the solar s-process pattern (dotted line) scaled to the Ba or Sr abundance of each star. The r- and s- fractions are from Arlandini et al. (1999), except for Th and U which are from Burris et al. (2000).
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