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A study of be stars in the magellanic clouds

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Iqbal, Shaheen; Keller, Stefan

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We present the results of a photometric survey for Be stars in 11 young clusters in the Large Magellanic Cloud and 14 young clusters in the Small Magellanic Cloud. B stars with hydrogen in emission are identified on the basis of their R-Hα colour. We fin

dc.contributor.authorIqbal, Shaheen
dc.contributor.authorKeller, Stefan
dc.date.accessioned2015-12-13T22:31:22Z
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/75219
dc.description.abstractWe present the results of a photometric survey for Be stars in 11 young clusters in the Large Magellanic Cloud and 14 young clusters in the Small Magellanic Cloud. B stars with hydrogen in emission are identified on the basis of their R-Hα colour. We fin
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Be-Magellanic clouds; Stars: early-type; Stars: emission-line
dc.titleA study of be stars in the magellanic clouds
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume435
dc.date.issued2013
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB4521
local.type.statusPublished Version
local.contributor.affiliationIqbal, Shaheen, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationKeller, Stefan, College of Physical and Mathematical Sciences, ANU
local.description.embargo2037-12-31
local.bibliographicCitation.issue4
local.bibliographicCitation.startpage3103
local.bibliographicCitation.lastpage3110
local.identifier.doi10.1093/mnras/stt1502
dc.date.updated2016-02-24T09:26:02Z
local.identifier.scopusID2-s2.0-84885807369
local.identifier.thomsonID000325774700026
CollectionsANU Research Publications

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