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Pulsating stars in NGC 6231: Frequency analysis and photometric mode identification near the main-sequence

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dc.contributor.authorMeingast, S
dc.contributor.authorHandler, G
dc.contributor.authorShobbrook, R
dc.date.accessioned2015-12-13T22:32:31Z
dc.date.issued2013
dc.date.updated2015-12-11T09:08:14Z
dc.description.abstractAims. We used Johnson UBV photometric CCD observations to identify pulsating and other variable stars in the young open cluster NGC 6231. The multi-colour information was used to classify pulsating variables, perform frequency analysis, and, where possibl
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/75601
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.titlePulsating stars in NGC 6231: Frequency analysis and photometric mode identification near the main-sequence
dc.typeJournal article
local.contributor.affiliationMeingast, S, Institut für Astrophysik, Universität Wien
local.contributor.affiliationHandler, G, Copernicus Astronomical Center
local.contributor.affiliationShobbrook, R, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidShobbrook, R, u4010450
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB4696
local.identifier.citationvolume559
local.identifier.doi10.1051/0004-6361/201220823
local.identifier.scopusID2-s2.0-84888213879
local.type.statusPublished Version

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