Publication:
Can Uranus and Neptune form concurrently via pebble, gas, and planetesimal accretion?

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cris.virtual.author-orcid0000-0002-8929-4660
cris.virtualsource.author-orcidff2d55a8-0f53-4d45-8d72-6ef5c6ee4b17
dc.contributor.authorEriksson, Linn E J
dc.contributor.authorMol Lous, Marit Anne Sylvie
dc.contributor.authorShibata, Sho
dc.contributor.authorHelled, Ravit
dc.date.accessioned2024-12-13T16:01:03Z
dc.date.available2024-12-13T16:01:03Z
dc.date.issued2023-12
dc.description.numberOfPages17
dc.description.sponsorshipNCCR PlanetS Universität Bern
dc.identifier.doi10.48350/187905
dc.identifier.publisherDOI10.1093/mnras/stad3007
dc.identifier.urihttps://boris-portal.unibe.ch/handle/20.500.12422/193967
dc.language.isoen
dc.publisherOxford University Press
dc.relation.ispartofMonthly notices of the Royal Astronomical Society
dc.relation.issn0035-8711
dc.relation.organizationDCD5A442C44AE17DE0405C82790C4DE2
dc.relation.organizationF741DD9E19B03C32E043960C5C82F84E
dc.relation.organizationDCD5A442BE9BE17DE0405C82790C4DE2
dc.subject.ddc500 - Science::530 - Physics
dc.titleCan Uranus and Neptune form concurrently via pebble, gas, and planetesimal accretion?
dc.typearticle
dspace.entity.typePublication
dspace.file.typetext
oaire.citation.endPage4876
oaire.citation.issue4
oaire.citation.startPage4860
oaire.citation.volume526
oairecerif.author.affiliationNCCR PlanetS Universität Bern
oairecerif.author.affiliation2Physikalisches Institut der Universität Bern
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unibe.contributor.rolecreator
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unibe.date.licenseChanged2023-10-27 13:43:49
unibe.description.ispublishedpub
unibe.eprints.legacyId187905
unibe.refereedTRUE
unibe.subtype.articlejournal

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