dc.contributor.author | Brugger, N | en_US |
dc.contributor.author | Burn, R | en_US |
dc.contributor.author | Coleman, GAL | en_US |
dc.contributor.author | Alibert, Y | en_US |
dc.contributor.author | Benz, W | en_US |
dc.date.accessioned | 2020-08-24T08:45:57Z | |
dc.date.available | 2020-06-06 | en_US |
dc.date.issued | 2020-08-03 | en_US |
dc.identifier.issn | 0004-6361 | en_US |
dc.identifier.other | ARTN A21 | en_US |
dc.identifier.uri | https://qmro.qmul.ac.uk/xmlui/handle/123456789/66540 | |
dc.relation.ispartof | ASTRONOMY & ASTROPHYSICS | en_US |
dc.rights | This 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.subject | planet-disk interactions | en_US |
dc.subject | planets and satellites | en_US |
dc.subject | formation | en_US |
dc.subject | planets and satellites | en_US |
dc.subject | physical evolution | en_US |
dc.subject | planets and satellites | en_US |
dc.subject | gaseous planets | en_US |
dc.subject | planets and satellites | en_US |
dc.subject | terrestrial planets | en_US |
dc.title | Pebbles versus planetesimals The outcomes of population synthesis models | en_US |
dc.type | Article | |
dc.rights.holder | © 2020 The European Southern Observatory (ESO) | |
dc.identifier.doi | 10.1051/0004-6361/202038042 | en_US |
pubs.author-url | http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000559309100003&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6a | en_US |
pubs.notes | Not known | en_US |
pubs.publication-status | Published | en_US |
pubs.volume | 640 | en_US |
rioxxterms.funder | Default funder | en_US |
rioxxterms.identifier.project | Default project | en_US |