Photometry of Gs UMa: A suspected ? Scuti variable

dc.contributor.authorKahraman Aliçavuş, F.
dc.contributor.authorRaheem, A.
dc.contributor.authorÇoban, G.Ç.
dc.contributor.authorTambulut, E.M.
dc.contributor.authorGögülter, Ü.
dc.contributor.authorBaş, L.
dc.contributor.authorÇevirici, B.
dc.date.accessioned2025-01-27T18:59:00Z
dc.date.available2025-01-27T18:59:00Z
dc.date.issued2018
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractWe present the time series analysis of GS UMa. GS UMa is a suspected ? Scuti variable with a primary frequency of 6.0987 d-1. © 2018.
dc.identifier.doi10.22444/IBVS.6246
dc.identifier.issn0374-0676
dc.identifier.issue6246
dc.identifier.scopus2-s2.0-85056564782
dc.identifier.scopusqualityN/A
dc.identifier.urihttps://doi.org/10.22444/IBVS.6246
dc.identifier.urihttps://hdl.handle.net/20.500.12428/13112
dc.identifier.volume63
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherHungarian Academy of Sciences (Konkoly Observatory)
dc.relation.ispartofInformation Bulletin on Variable Stars
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_Scopus_20250125
dc.titlePhotometry of Gs UMa: A suspected ? Scuti variable
dc.typeArticle

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