An inhomogeneous model for the Galactic halo: a possible explanation for the spread observed in s- and r-process elements

Publisher： Edp Sciences

E-ISSN： 1432-0746|481|3|691-699

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.481, Iss.3, 2008-04, pp. : 691-699

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

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