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Helium enhanced stars and multiple populations along the horizontal branch of NGC 2808: Direct spectroscopic measurements

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dc.contributor.authorMarino, Anna
dc.contributor.authorMilone, Antonino
dc.contributor.authorPrzybilla, N
dc.contributor.authorBergemann, Maria
dc.contributor.authorLind, K.
dc.contributor.authorAsplund, Martin
dc.contributor.authorCassisi, S
dc.contributor.authorCatelan, M
dc.contributor.authorCasagrande, Luca
dc.contributor.authorValcarce, A.A.R
dc.contributor.authorBedin, L R
dc.contributor.authorCortes, C
dc.contributor.authorD'Antona, Francesca
dc.contributor.authorJerjen, Helmut
dc.contributor.authorPiotto, G
dc.contributor.authorSchlesinger, Katharine
dc.contributor.authorZoccali, M
dc.contributor.authorAngeloni, R
dc.date.accessioned2015-12-13T22:39:45Z
dc.date.issued2013
dc.date.updated2015-12-11T09:52:04Z
dc.description.abstractWe present an abundance analysis of 96 horizontal branch (HB) stars in NGC 2808, a globularcluster exhibiting a complex multiple stellar population pattern. These stars are distributed indifferent portions of the HB and cover a wide range of temperature.
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/77918
dc.publisherBlackwell Publishing Ltd
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.titleHelium enhanced stars and multiple populations along the horizontal branch of NGC 2808: Direct spectroscopic measurements
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage1627
local.bibliographicCitation.startpage1609
local.contributor.affiliationMarino, Anna, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMilone, Antonino, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationPrzybilla, N, University of Innsbruck
local.contributor.affiliationBergemann, Maria, Max Planck Institut fur Astrophysik
local.contributor.affiliationLind, K., University of Cambridge
local.contributor.affiliationAsplund, Martin, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationCassisi, S, Osservatorio Astronomico di Teramo
local.contributor.affiliationCatelan, M, Pontificia Universidad Catolica de Chile
local.contributor.affiliationCasagrande, Luca, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationValcarce, A.A.R, Universidade Federal do Rio Grande do Norte
local.contributor.affiliationBedin, L R, INAF-Osservatorio Astronomico di Padova
local.contributor.affiliationCortes, C, Universidad Metropolitana de Ciencias de la Edicacion
local.contributor.affiliationD'Antona, Francesca, INAF-Osservatorio Astronomico di Roma
local.contributor.affiliationJerjen, Helmut, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationPiotto, G, Università di Padova
local.contributor.affiliationSchlesinger, Katharine, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationZoccali, M, Universidad Catolica de Chile
local.contributor.affiliationAngeloni, R, Universidad Catolica de Chile
local.contributor.authoruidMarino, Anna, u5239722
local.contributor.authoruidMilone, Antonino, u5219567
local.contributor.authoruidAsplund, Martin, u4042723
local.contributor.authoruidCasagrande, Luca, u5209059
local.contributor.authoruidJerjen, Helmut, u9611777
local.contributor.authoruidSchlesinger, Katharine, u5239304
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB6651
local.identifier.citationvolume437
local.identifier.doi10.1093/mnras/stt1993
local.identifier.scopusID2-s2.0-84890895962
local.identifier.thomsonID000331617000044
local.type.statusPublished Version

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