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The Helium Abundances of &omega Centauri

Norris, John

Description

Recent Hubble Space Telescope color magnitude diagrams (CMDs) of ω Centauri, which clearly show three sequences in the region of the main-sequence turnoff together with a double lower main sequence, are explained in terms of three populations having cano

dc.contributor.authorNorris, John
dc.date.accessioned2015-12-13T23:10:10Z
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/87331
dc.description.abstractRecent Hubble Space Telescope color magnitude diagrams (CMDs) of ω Centauri, which clearly show three sequences in the region of the main-sequence turnoff together with a double lower main sequence, are explained in terms of three populations having cano
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.titleThe Helium Abundances of &omega Centauri
dc.typeJournal article
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.citationvolume612
dc.date.issued2004
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub16570
local.type.statusPublished Version
local.contributor.affiliationNorris, John, College of Physical and Mathematical Sciences, ANU
local.description.embargo2037-12-31
local.bibliographicCitation.startpageL25
local.bibliographicCitation.lastpageL28
local.identifier.doi10.1086/423986
dc.date.updated2015-12-12T08:22:36Z
local.identifier.scopusID2-s2.0-8744229642
CollectionsANU Research Publications

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