The AGB stars of the intermediate-age LMC cluster NGC 1846 - Variability and age determination

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dc.contributor.authorLebzelter, Thomas
dc.contributor.authorWood, Peter R
dc.date.accessioned2015-12-10T22:23:08Z
dc.date.issued2007
dc.date.updated2015-12-09T09:05:02Z
dc.description.abstractAims. We investigate variability and we model the pulsational behaviour of AGB variables in the intermediate-age LMC cluster NGC 1846. Methods. Our own photometric monitoring has been combined with data from the MACHO archive to detect 22 variables among
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/52652
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Carbon; Galaxies; Mathematical models; Opacity; Parameter estimation; Photometry; Galaxy: globular clusters; Pulsational behaviours; Stars Galaxy: globular clusters: individual: NGC 1846; Stars: AGB and post-AGB; Stars: variables: general
dc.titleThe AGB stars of the intermediate-age LMC cluster NGC 1846 - Variability and age determination
dc.typeJournal article
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage653
local.bibliographicCitation.startpage643
local.contributor.affiliationLebzelter, Thomas, University of Vienna
local.contributor.affiliationWood, Peter R, College of Physical and Mathematical Sciences, ANU
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.ariespublicationU1408929xPUB252
local.identifier.citationvolume475
local.identifier.doi10.1051/0004-6361:20078395
local.identifier.scopusID2-s2.0-36549066185
local.type.statusPublished Version

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