The helium spread in the globular cluster 47 Tuc

dc.contributor.authorDi Criscienzo, M
dc.contributor.authorVentura, P
dc.contributor.authorD'Antona, Francesca
dc.contributor.authorMilone, Antonino
dc.contributor.authorPiotto, G
dc.date.accessioned2015-12-13T22:45:04Z
dc.date.issued2010
dc.date.updated2016-02-24T09:38:46Z
dc.description.abstractSpectroscopy has shown the presence of CN band dichotomy and Na-O anticorrelations for 50-70 per cent of the investigated samples in the cluster 47 Tuc, otherwise considered a 'normal' prototype of high-metallicity clusters from its photometric analysis.
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/79587
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Globular clusters: general; Globular clusters: individual: 47 Tuc; Stars: evolution; Stars: horizontal branch
dc.titleThe helium spread in the globular cluster 47 Tuc
dc.typeJournal article
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage1005
local.bibliographicCitation.startpage999
local.contributor.affiliationDi Criscienzo, M, INAF - Osservatorio Astronomico di Roma
local.contributor.affiliationVentura, P, INAF-Osservatorio Astronomico di Roma
local.contributor.affiliationD'Antona, Francesca, INAF-Osservatorio Astronomico di Roma
local.contributor.affiliationMilone, Antonino, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationPiotto, G, Università di Padova
local.contributor.authoremailu5219567@anu.edu.au
local.contributor.authoruidMilone, Antonino, u5219567
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationf5625xPUB7998
local.identifier.citationvolume408
local.identifier.doi10.1111/j.1365-2966.2010.17168.x
local.identifier.scopusID2-s2.0-78649396833
local.identifier.uidSubmittedByf5625
local.type.statusPublished Version

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