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Late-type giant variables in NGC 6522, LMC and SMC. How do they differ?

dc.contributor.authorSchultheis, M.
dc.contributor.authorGlass, I.
dc.contributor.authorCioni, M-R.L.
dc.date.accessioned2008-07-14T12:24:21Z
dc.date.available2008-07-14T12:24:21Z
dc.date.issued2004
dc.identifier.citationSchultheis , M , Glass , I & Cioni , M-RL 2004 , ' Late-type giant variables in NGC 6522, LMC and SMC. How do they differ? ' , Astronomy and Astrophysics , vol. 427 , pp. 945-958 . https://doi.org/10.1051/0004-6361:20041454
dc.identifier.issn0004-6361
dc.identifier.otherdspace: 2299/2210
dc.identifier.urihttp://hdl.handle.net/2299/2210
dc.descriptionOriginal article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory
dc.format.extent2159425
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.titleLate-type giant variables in NGC 6522, LMC and SMC. How do they differ?en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1051/0004-6361:20041454
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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