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dc.contributor.authorDobbs, Clare
dc.date.accessioned2024-04-15T12:16:28Z
dc.date.issued2024-04-15
dc.date.updated2024-04-13T15:42:53Z
dc.description.abstractThis is the dataset used for the Dobbs et al. (2018) article "Simulations of the flocculent spiral M33: what drives the spiral structure?" published in Monthly Notices of the Royal Astronomical Society.en_GB
dc.description.sponsorshipEuropean Research Council (ERC)en_GB
dc.identifier.doi10.24378/exe.5127
dc.identifier.urihttp://hdl.handle.net/10871/135746
dc.language.isoenen_GB
dc.publisherUniversity of Exeteren_GB
dc.relation.urlhttp://hdl.handle.net/10871/34891en_GB
dc.rightsPlease email Clare Dobbs before using this data.en_GB
dc.subjectgalaxies: individual: M33en_GB
dc.subjectISM: generalen_GB
dc.subjectgalaxies: spiralen_GB
dc.titleSimulations of the flocculent spiral M33: what drives the spiral structure? (dataset)en_GB
dc.typeDataseten_GB
dc.date.available2024-04-15T12:16:28Z
dc.descriptionThese are the datasets from the medium feedback, high feedback and high resolution runs from Dobbs et al. 2018, on simulations of the galaxy M33. To view files, use the program splash (http://users.monash.edu.au/~dprice/splash/).en_GB
dc.descriptionThe article associated with this dataset is available in ORE at: http://hdl.handle.net/10871/34891en_GB
dc.rights.urihttp://www.rioxx.net/licenses/all-rights-reserveden_GB
rioxxterms.versionNAen_GB
rioxxterms.typeOtheren_GB
refterms.dateFOA2024-04-15T12:16:35Z


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