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Photometric study of two β Cephei pulsators in eclipsing systems

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dc.contributor.authorDrobek, D
dc.contributor.authorPigulski, A
dc.contributor.authorShobbrook, R
dc.contributor.authorNarwid, A
dc.date.accessioned2015-12-10T22:39:23Z
dc.date.issued2010
dc.date.updated2016-02-24T08:28:10Z
dc.description.abstractWe present results of a photometric study of the young southern open cluster Stock 14. This cluster is known to contain two eclipsing systems with presumed β Cephei components, HD 101794 and HD 101838. We confirm variability due to pulsations and eclipse
dc.identifier.issn0004-6337
dc.identifier.urihttp://hdl.handle.net/1885/57148
dc.publisherWiley-VCH Verlag GMBH
dc.sourceAstronomische Nachrichten
dc.subjectKeywords: Binaries: eclipsing; Open clusters and associations: individual (Stock 14); Stars: individual (HD 101794, HD 101838); Stars: oscillations; Techniques: photometric
dc.titlePhotometric study of two β Cephei pulsators in eclipsing systems
dc.typeJournal article
local.bibliographicCitation.issue9-10
local.bibliographicCitation.lastpage1079
local.bibliographicCitation.startpage1077
local.contributor.affiliationDrobek, D, Instytut Astronomiczny Uniwersytetu Wroławskiego
local.contributor.affiliationPigulski, A, Wroclaw University Observatory
local.contributor.affiliationShobbrook, R, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationNarwid, A, Instytut Astronomiczny Uniwersytetu Wroławskiego
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.ariespublicationf2965xPUB389
local.identifier.citationvolume331
local.identifier.doi10.1002/asna.201011461
local.identifier.scopusID2-s2.0-78649409606
local.type.statusPublished Version

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