Setting the stage: Planet formation and volatile delivery

dc.creatorVenturini, Julia
dc.creatorRonco, María Paula
dc.creatorGuilera, Octavio Miguel
dc.date.accessioned2021-11-02T12:16:33Z
dc.date.accessioned2022-10-15T08:17:53Z
dc.date.available2021-11-02T12:16:33Z
dc.date.available2022-10-15T08:17:53Z
dc.date.created2021-11-02T12:16:33Z
dc.date.issued2020-07-01
dc.identifierVenturini, Julia; Ronco, María Paula; Guilera, Octavio Miguel; Setting the stage: Planet formation and volatile delivery; Springer; Space Science Reviews; 216; 5; 01-7-2020; 1-32
dc.identifier0038-6308
dc.identifierhttp://hdl.handle.net/11336/145696
dc.identifier1572-9672
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4364219
dc.description.abstractThe diversity in mass and composition of planetary atmospheres stems from the different building blocks present in protoplanetary discs and from the different physical and chemical processes that these experience during the planetary assembly and evolution. This review aims to summarise, in a nutshell, the key concepts and processes operating during planet formation, with a focus on the delivery of volatiles to the inner regions of the planetary system.
dc.languageeng
dc.publisherSpringer
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://link.springer.com/10.1007/s11214-020-00700-y
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1007/s11214-020-00700-y
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectEXOPLANETS
dc.subjectPLANET FORMATION
dc.subjectSOLAR SYSTEM
dc.subjectVOLATILE DELIVERY
dc.titleSetting the stage: Planet formation and volatile delivery
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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