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dc.contributor.advisorDownes, Turlough
dc.contributor.advisorScholz, Aleks
dc.contributor.advisorRay, Tom
dc.contributor.authorRodgers-Lee, Donna
dc.date.accessioned2024-11-22T18:10:40Z
dc.date.available2024-11-22T18:10:40Z
dc.date.issued2017
dc.identifier.citationDonna Rodgers-Lee, 'Star formation : protoplanetary disk evolution', [thesis], Trinity College (Dublin, Ireland). School of Physics, 2017, pp 226
dc.identifier.otherTHESIS 11498
dc.description.abstractThis thesis focuses on the evolution of protoplanetary disks around young stellar objects using a combination of observations and simulations. Understanding protoplanetary disk evolution impacts theories of planet formation and how the solar system might have formed. The physical processes in protoplanetary disks are likely to occur in many astrophysical accretion disks, hence studying protoplanetary disk evolution can influence accretion disk theory in general.
dc.format1 volume
dc.language.isoen
dc.publisherTrinity College (Dublin, Ireland). School of Physics
dc.relation.isversionofhttp://stella.catalogue.tcd.ie/iii/encore/record/C__Rb17321197
dc.subjectPhysics, Ph.D.
dc.subjectPhD Trinity College Dublin, 2017
dc.titleStar formation : protoplanetary disk evolution
dc.typethesis
dc.type.supercollectionthesis_dissertations
dc.type.supercollectionrefereed_publications
dc.type.qualificationlevelDoctoral
dc.type.qualificationnameDoctor of Philosophy (Ph.D.)
dc.rights.ecaccessrightsopenAccess
dc.format.extentpaginationpp 226
dc.description.noteTARA (Trinity's Access to Research Archive) has a robust takedown policy. Please contact us if you have any concerns: rssadmin@tcd.ie
dc.identifier.urihttps://hdl.handle.net/2262/110357


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