Explaining the Ba, Y, Sr, and Eu abundance scatter in metal-poor halo stars: constraints to the r-process

Author: Cescutti G.   Chiappini C.  

Publisher: Edp Sciences

E-ISSN: 1432-0746|565|issue|A51-A51

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.565, Iss.issue, 2014-05, pp. : A51-A51

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Abstract