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dc.contributor.authorCottenier S.
dc.contributor.authorProbert M. I. J.
dc.contributor.authorVan Hoolst T.
dc.contributor.authorVan Speybroeck V.
dc.contributor.authorWaroquier M.
dc.date12/2011
dc.date.accessioned2016-04-13T10:04:28Z
dc.date.available2016-04-13T10:04:28Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3543
dc.descriptionhttp://esoads.eso.org/abs/2011E%26PSL.312..237C
dc.languageeng
dc.rightsRestricted Access
dc.titleCrystal structure prediction for iron as inner core material in heavy terrestrial planets
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleEarth and Planetary Science Letters
dc.source.volume312
dc.source.page237
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/j.epsl.2011.09.045
dc.identifier.urlhttp://esoads.eso.org/abs/2011E%26PSL.312..237C
dc.source.editorELSEVIER


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