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Geometry of the Large Magellanic Cloud Disk: Results from MACHO and the Two Micron All Sky Survey

dc.contributor.authorKeller, Stefan
dc.contributor.authorNikolaev, Sergei
dc.contributor.authorDrake, Andrew J
dc.contributor.authorCook, Kem H
dc.contributor.authorDalal, N
dc.contributor.authorGriest, K
dc.contributor.authorWelch, D L
dc.contributor.authorKanbur, S
dc.date.accessioned2015-12-07T22:16:51Z
dc.date.issued2004
dc.date.updated2015-12-07T07:57:53Z
dc.description.abstractWe present a detailed study of the viewing angles and geometry of the inner LMC (ρ ≲ 4°) based on a sample of more than 2000 MACHO Cepheids with complete {VR}KC light curves and single-phase Two Micron All Sky Survey (2MASS) JHKS observations. The sam
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/18236
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Cepheids; Dust, extinction; Galaxies: individual (Large Magellanic Cloud) galaxies: structure
dc.titleGeometry of the Large Magellanic Cloud Disk: Results from MACHO and the Two Micron All Sky Survey
dc.typeJournal article
local.bibliographicCitation.lastpage276
local.bibliographicCitation.startpage260
local.contributor.affiliationKeller, Stefan, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationNikolaev, Sergei, Lawrence Livermore National Laboratory
local.contributor.affiliationDrake, Andrew J, Pontifica Universidad Catolica
local.contributor.affiliationCook, Kem H, Lawrence Livermore National Laboratory
local.contributor.affiliationDalal, N, University of California
local.contributor.affiliationGriest, K, University of California
local.contributor.affiliationWelch, D L, McMaster University
local.contributor.affiliationKanbur, S, University of Massachusetts
local.contributor.authoruidKeller, Stefan, u9702857
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationu9702857xPUB3
local.identifier.citationvolume601
local.identifier.doi10.1086/380439
local.identifier.scopusID2-s2.0-1642633365
local.type.statusPublished Version

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