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dc.contributor.authorGressel, Oen_US
dc.contributor.authorNelson, RPen_US
dc.contributor.authorTurner, NJen_US
dc.date.accessioned2015-05-20T11:38:21Z
dc.date.issued2011-08en_US
dc.identifier.issn0035-8711en_US
dc.identifier.urihttp://mnras.oxfordjournals.org/content/415/4/3291
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/7464
dc.description.sponsorship. NJT was supported by the Jet Propulsion Laboratory, California Institute of Technology, the NASA Origins and Outer Planets programs, and the Alexander von Humboldt Foundation.en_US
dc.format.extent3291 - 3307en_US
dc.language.isoenen_US
dc.relation.ispartofMON NOT R ASTRON SOCen_US
dc.subjectaccretion, accretion discsen_US
dc.subjectMHDen_US
dc.subjectmethods: numericalen_US
dc.subjectprotoplanetary discsen_US
dc.subject3-DIMENSIONAL MAGNETOHYDRODYNAMIC SIMULATIONSen_US
dc.subjectSHEARING BOX APPROXIMATIONen_US
dc.subjectWEAKLY MAGNETIZED DISKSen_US
dc.subjectSPIRAL DENSITY WAVESen_US
dc.subjectMRI CHANNEL FLOWSen_US
dc.subjectX-RAY IONIZATIONen_US
dc.subjectACCRETION DISKSen_US
dc.subjectPROTOSTELLAR DISKSen_US
dc.subjectMAGNETOROTATIONAL INSTABILITYen_US
dc.subjectPLANET FORMATIONen_US
dc.titleOn the dynamics of planetesimals embedded in turbulent protoplanetary discs with dead zonesen_US
dc.typeArticle
dc.identifier.doi10.1111/j.1365-2966.2011.18944.xen_US
pubs.issue4en_US
pubs.notesNot knownen_US
pubs.organisational-group/Queen Mary University of London
pubs.organisational-group/Queen Mary University of London/Faculty of Science & Engineering
pubs.organisational-group/Queen Mary University of London/Faculty of Science & Engineering/Mathematical Sciences - Staff and Research Students
pubs.organisational-group/Queen Mary University of London/Faculty of Science & Engineering/Physics and Astronomy
pubs.volume415en_US


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