The pulsation of AGB stars in the Magellanic Cloud clusters NGC 1978 and 419

dc.contributor.authorKamath, Devika
dc.contributor.authorWood, Peter R
dc.contributor.authorSoszyński, Igor
dc.contributor.authorLebzelter, Thomas
dc.date.accessioned2015-12-10T22:39:33Z
dc.date.issued2010
dc.date.updated2016-02-24T08:28:11Z
dc.description.abstractThe intermediate-age Magellanic Cloud clusters NGC 1978 and 419 are each found to contain substantial numbers of pulsating asymptotic giant branch (AGB) stars, both oxygen rich and carbon rich. Each cluster also contains two pulsating AGB stars which are
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/57230
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Galaxies: star clusters: individual: NGC 1978; Galaxies: star clusters: individual: NGC 419; Magellanic Clouds; Stars: AGB and post-AGB; Stars: mass-loss; Stars: variables: general
dc.titleThe pulsation of AGB stars in the Magellanic Cloud clusters NGC 1978 and 419
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage534
local.bibliographicCitation.startpage522
local.contributor.affiliationKamath, Devika, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWood, Peter R, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSoszyński, Igor, Warsaw University Observatory
local.contributor.affiliationLebzelter, Thomas, University of Vienna
local.contributor.authoruidKamath, Devika, u4602544
local.contributor.authoruidWood, Peter R, u7900259
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf2965xPUB392
local.identifier.citationvolume408
local.identifier.doi10.1111/j.1365-2966.2010.17137.x
local.identifier.scopusID2-s2.0-78649427566
local.identifier.thomsonID000283118100041
local.type.statusPublished Version

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