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dc.contributor.authorBrugger, Nen_US
dc.contributor.authorBurn, Ren_US
dc.contributor.authorColeman, GALen_US
dc.contributor.authorAlibert, Yen_US
dc.contributor.authorBenz, Wen_US
dc.date.accessioned2020-08-24T08:45:57Z
dc.date.available2020-06-06en_US
dc.date.issued2020-08-03en_US
dc.identifier.issn0004-6361en_US
dc.identifier.otherARTN A21en_US
dc.identifier.urihttps://qmro.qmul.ac.uk/xmlui/handle/123456789/66540
dc.relation.ispartofASTRONOMY & ASTROPHYSICSen_US
dc.rightsThis is a pre-copyedited, author-produced version of an article accepted for publication in Astronomy and Astrophysics following peer review. The version of record is available https://www.aanda.org/articles/aa/abs/2020/08/aa38042-20/aa38042-20.html
dc.subjectplanet-disk interactionsen_US
dc.subjectplanets and satellitesen_US
dc.subjectformationen_US
dc.subjectplanets and satellitesen_US
dc.subjectphysical evolutionen_US
dc.subjectplanets and satellitesen_US
dc.subjectgaseous planetsen_US
dc.subjectplanets and satellitesen_US
dc.subjectterrestrial planetsen_US
dc.titlePebbles versus planetesimals The outcomes of population synthesis modelsen_US
dc.typeArticle
dc.rights.holder© 2020 The European Southern Observatory (ESO)
dc.identifier.doi10.1051/0004-6361/202038042en_US
pubs.author-urlhttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000559309100003&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6aen_US
pubs.notesNot knownen_US
pubs.publication-statusPublisheden_US
pubs.volume640en_US
rioxxterms.funderDefault funderen_US
rioxxterms.identifier.projectDefault projecten_US


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