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Chemical abundances in globular clusters

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dc.contributor.authorYong, David
dc.coverage.spatialCairns Australia
dc.date.accessioned2015-12-13T22:56:26Z
dc.date.createdAugust 5-12 2012
dc.date.issued2013
dc.date.updated2015-12-11T11:15:35Z
dc.description.abstractThe Milky Way globular clusters are ideal laboratories for testing the predictions of nuclear astrophysics. Driven by Hubble Space Telescope photometry and high-resolution multi-object spectro-graphs on 8m-class telescopes, the study of chemical abundance
dc.identifier.urihttp://hdl.handle.net/1885/82797
dc.publisherConference Organising Committee
dc.relation.ispartofseries12th International Symposium on Nuclei in the Cosmos, NIC 2012
dc.sourceProceedings of Science
dc.titleChemical abundances in globular clusters
dc.typeConference paper
local.contributor.affiliationYong, David, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidYong, David, u3207952
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB11001
local.identifier.scopusID2-s2.0-84887485498
local.type.statusPublished Version

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