dc.date.accessioned2020-03-11T20:26:50Z
dc.date.accessioned2022-10-18T22:41:40Z
dc.date.available2020-03-11T20:26:50Z
dc.date.available2022-10-18T22:41:40Z
dc.date.created2020-03-11T20:26:50Z
dc.date.issued2015
dc.identifierhttp://hdl.handle.net/10533/238118
dc.identifier15090013
dc.identifierWOS:000359013400009
dc.identifierno scielo
dc.identifiereid=2-s2.0-84934760862
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4469457
dc.description.abstractKiruna-type iron oxide–apatite (IOA) deposits are an important source of Fe ore, and two radically different processes are being actively investigated for their origin. One hypothesis invokes direct crystallization of immiscible Fe-rich melt that separate
dc.languageeng
dc.relationhttps://doi.org/10.1130/G36650.1
dc.relation10.1130/G36650.1
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleGiant Kiruna-type deposits form by efficient flotation of magmatic magnetite suspensions
dc.typeArticulo


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