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Multiple stellar populations in Magellanic Cloud clusters: II. Evidence also in the young NGC 1844?

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dc.contributor.authorMilone, Antonino
dc.contributor.authorBedin, L R
dc.contributor.authorCassisi, S
dc.contributor.authorPiotto, G
dc.contributor.authorAnderson, Jay
dc.contributor.authorPietrinferni, A
dc.contributor.authorBuonanno, R
dc.date.accessioned2015-12-13T22:29:20Z
dc.date.issued2013
dc.date.updated2016-02-24T09:23:00Z
dc.description.abstractWe used Hubble Space Telescope observations to study the young cluster NGC 1844 in the Large Magellanic Cloud (LMC). We estimated the fraction and the mass-ratio distribution of photometric binaries and report that the main sequence presents an intrinsic
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/74654
dc.publisherSpringer
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Binaries: general; Globular clusters: individual; Hubble space telescopes; Large magellanic clouds; Magellanic Clouds; Stars: Population II; Stellar populations; Stellar rotation; Galaxies; Helium; Photometry; Stars Binaries: general; Globular clusters: individual: NGC 1844; Magellanic Clouds; Stars: Population II
dc.titleMultiple stellar populations in Magellanic Cloud clusters: II. Evidence also in the young NGC 1844?
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.startpage10
local.contributor.affiliationMilone, Antonino, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBedin, L R, INAF-Osservatorio Astronomico di Padova
local.contributor.affiliationCassisi, S, Osservatorio Astronomico di Teramo
local.contributor.affiliationPiotto, G, Università di Padova
local.contributor.affiliationAnderson, Jay, Space Telescope Science Institute
local.contributor.affiliationPietrinferni, A, INAF - Osservatorio Astronomico di Teramo
local.contributor.affiliationBuonanno, R, INAF – Osservatorio Astronomico di Collurania
local.contributor.authoruidMilone, Antonino, u5219567
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB4225
local.identifier.citationvolume555
local.identifier.doi10.1051/0004-6361/201220567
local.identifier.scopusID2-s2.0-84880677043
local.identifier.thomsonID000322008600143
local.type.statusPublished Version

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