dc.contributor.author | Coleman, GAL | en_US |
dc.contributor.author | Nelson, RP | en_US |
dc.contributor.author | Paardekooper, SJ | en_US |
dc.contributor.author | Dreizler, S | en_US |
dc.contributor.author | Giesers, B | en_US |
dc.contributor.author | Anglada-Escude, G | en_US |
dc.date.accessioned | 2017-03-08T14:16:05Z | |
dc.date.available | 2016-09-20 | en_US |
dc.date.issued | 2017-05 | en_US |
dc.date.submitted | 2017-02-28T09:54:34.469Z | |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://qmro.qmul.ac.uk/xmlui/handle/123456789/19729 | |
dc.format.extent | 996 - 1007 | en_US |
dc.relation.ispartof | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.subject | planets and satellites: dynamical evolution and stability | en_US |
dc.subject | planets and satellites: formation | en_US |
dc.subject | planet-disc interactions | en_US |
dc.subject | planetary systems | en_US |
dc.title | Exploring plausible formation scenarios for the planet candidate orbiting Proxima Centauri | en_US |
dc.type | Article | |
dc.rights.holder | © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society | |
dc.identifier.doi | 10.1093/mnras/stx169 | en_US |
pubs.author-url | http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000398418900070&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6a | en_US |
pubs.issue | 1 | en_US |
pubs.notes | No embargo | en_US |
pubs.publication-status | Published | en_US |
pubs.volume | 467 | en_US |
qmul.funder | Astronomy Research at Queen Mary::Science and Technology Facilities Council | en_US |