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dc.contributor.authorCioni, M-R.L.
dc.contributor.editorSpinoglio, L.
dc.contributor.editorEpchtein, N.
dc.date.accessioned2011-11-21T15:01:13Z
dc.date.available2011-11-21T15:01:13Z
dc.date.issued2010
dc.identifier.citationCioni , M-RL 2010 , IR imaging surveys of AGB stars in the Magellanic Clouds . in L Spinoglio & N Epchtein (eds) , Procs 3rd Arena Conference : An Astronomical Observatory at CONCORDIA . EAS Publications Series , vol. 40 , European Astronomical Society , pp. 137-145 . https://doi.org/10.1051/eas/1040019
dc.identifier.otherPURE: 455331
dc.identifier.otherPURE UUID: ca065355-6287-4d42-ab66-b2e498046814
dc.identifier.otherdspace: 2299/4188
dc.identifier.otherScopus: 73549111569
dc.identifier.urihttp://hdl.handle.net/2299/7051
dc.description“The original publication is available at www.edpsciences.org/eas”. Copyright EAS/EDP Sciences.
dc.description.abstractAGB stars are ideal IR targets because they are cool and bright. Most of them escaped detection in optical or shallow IR surveys in the eighties contributing to the puzzling missing number of AGB stars with respect to theoretical predictions and former stages of evolution. Observations and AGB models have advanced steadily in the following decades providing us with an almost complete view of the AGB stars in the Magellanic Clouds. Their properties are tracers of structure and chemistry across galaxies. New surveys will be able to fill-in the gaps, in terms of sensitivity and monitoring, providing new constraints for the formation and evolution of the Magellanic Clouds.en
dc.language.isoeng
dc.publisherEuropean Astronomical Society
dc.relation.ispartofProcs 3rd Arena Conference
dc.relation.ispartofseriesEAS Publications Series
dc.titleIR imaging surveys of AGB stars in the Magellanic Cloudsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1051/eas/1040019
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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