Globular clusters and their link with stellar populations in the Milky Way

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dc.contributor.authorYong, David
dc.contributor.editorRodriguez, José Miguel
dc.coverage.spatialUnited Kingdom
dc.date.accessioned2023-03-14T22:03:07Z
dc.date.createdAugust 2018
dc.date.issued2019
dc.date.updated2022-01-09T07:17:23Z
dc.description.abstractObservations of stellar chemical compositions enable us to identify connections between globular clusters and stellar populations in the Milky Way. In particular, chemical abundance ratios provide detailed insight into the chemical enrichment histories of star clusters and the field populations. For some elements, there are striking differences between field and cluster stars which reflect different nucleosynthetic processes and/or chemical evolution. The goal of this talk was to provide an overview of similarities and differences in chemical compositions between globular clusters and the Milky Way as well as highlighting a few areas for further examination.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn1743-9221en_AU
dc.identifier.urihttp://hdl.handle.net/1885/287046
dc.language.isoen_AUen_AU
dc.publisherCambridge University Pressen_AU
dc.relation.ispartofseriesWhy Galaxies Care About AGB Stars: A Continuing Challenge through Cosmic Timeen_AU
dc.rights© International Astronomical Union 2020en_AU
dc.sourceProceedings of the International Astronomical Unionen_AU
dc.subjectGalaxy: globular clusters: generalen_AU
dc.subjectstars: abundancesen_AU
dc.titleGlobular clusters and their link with stellar populations in the Milky Wayen_AU
dc.typeConference paperen_AU
local.bibliographicCitation.lastpage23en_AU
local.bibliographicCitation.startpage19en_AU
local.contributor.affiliationYong, David, College of Science, ANUen_AU
local.contributor.authoremailu3207952@anu.edu.auen_AU
local.contributor.authoruidYong, David, u3207952en_AU
local.description.embargo2099-12-31
local.description.notesImported from ARIESen_AU
local.description.refereedYes
local.identifier.absfor510104 - Galactic astronomyen_AU
local.identifier.absseo280120 - Expanding knowledge in the physical sciencesen_AU
local.identifier.ariespublicationa383154xPUB11782en_AU
local.identifier.doi10.1017/S1743921319007361en_AU
local.identifier.scopusID2-s2.0-85081989171
local.identifier.uidSubmittedBya383154en_AU
local.publisher.urlhttps://www.cambridge.org/en_AU
local.type.statusPublished Versionen_AU

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