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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3142
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dc.contributor.authorPrantzos, N-
dc.contributor.authorGoswami, A-
dc.date.accessioned2008-08-14T11:16:08Z-
dc.date.available2008-08-14T11:16:08Z-
dc.date.issued2001-05-
dc.identifier.citationNuclear Physics A, Vol. 688, No. 1 - 2, pp. 37 – 40en
dc.identifier.issn0375-9474-
dc.identifier.urihttp://hdl.handle.net/2248/3142-
dc.descriptionRestricted Access-
dc.format.extent3894 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherElsevieren
dc.relation.urihttp://dx.doi.org/10.1016/S0375-9474(01)00664-9en
dc.subjectChemical evolutionen
dc.subjectMilky Way haloen
dc.titleChemical evolution of the Milky Way halo and disken
dc.typeArticleen
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