Planet formation via pebble accretion in externally photoevaporating discs
dc.contributor.author | Qiao, L | en_US |
dc.contributor.author | Coleman, GAL | en_US |
dc.contributor.author | Haworth, TJ | en_US |
dc.date.accessioned | 2023-11-03T10:11:53Z | |
dc.date.available | 2023-03-24 | en_US |
dc.date.issued | 2023 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | https://qmro.qmul.ac.uk/xmlui/handle/123456789/91646 | |
dc.format.extent | 1939 - 1950 | en_US |
dc.relation.ispartof | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.rights | This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. | |
dc.rights | Attribution 3.0 United States | * |
dc.rights.uri | http://creativecommons.org/licenses/by/3.0/us/ | * |
dc.subject | planets and satellites: formation | en_US |
dc.subject | protoplanetary discs | en_US |
dc.subject | circumstellar matter | en_US |
dc.title | Planet formation via pebble accretion in externally photoevaporating discs | en_US |
dc.type | Article | |
dc.rights.holder | © 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. | |
dc.identifier.doi | 10.1093/mnras/stad944 | en_US |
pubs.author-url | https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000989553900011&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6a | en_US |
pubs.issue | 2 | en_US |
pubs.notes | Not known | en_US |
pubs.publication-status | Published | en_US |
pubs.volume | 522 | en_US |
rioxxterms.funder | Default funder | en_US |
rioxxterms.identifier.project | Default project | en_US |
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Except where otherwise noted, this item's license is described as This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.