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Accretion of Saturn’s mid-sized moons during the viscous spreading of young massive rings: Solving the paradox of silicate-poor rings versus silicate-rich moons

dc.contributor.authorCharnoz S.
dc.contributor.authorCrida A.
dc.contributor.authorCastillo-Rogez J. C.
dc.contributor.authorLainey V.
dc.contributor.authorDones L.
dc.contributor.authorKaratekin Ö.
dc.contributor.authorTobie G.
dc.contributor.authorMathis S.
dc.contributor.authorLe Poncin-Lafitte C.
dc.contributor.authorSalmon J.
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/3542
dc.descriptionhttp://esoads.eso.org/abs/2011Icar..216..535C
dc.languageeng
dc.rightsRestricted Access
dc.titleAccretion of Saturn’s mid-sized moons during the viscous spreading of young massive rings: Solving the paradox of silicate-poor rings versus silicate-rich moons
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleIcarus
dc.source.volume216
dc.source.page535
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/j.icarus.2011.09.017
dc.identifier.urlhttp://esoads.eso.org/abs/2011Icar..216..535C
dc.source.editorELSEVIER


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