The Light and Colour Variations of MM Her

Basit Öğe Kaydı
dc.contributor.authorTaş G.
dc.date.accessioned2019-10-27T00:26:35Z
dc.date.available2019-10-27T00:26:35Z
dc.date.issued1999
dc.departmentEge Üniversitesien_US
dc.description.abstractRS CVn type eclipsing binary MM Herculis have been observed using B, V, R filters in 1997 and obtained light and colour curves were examined together with the earlier 12 light and colour curves obtained between 1976 and 1997. It was seen that the system is bluer, while it is fainter. Such finding probably reveals the evolutionary effect of the photospheric bright facular structures surrounding starspots.en_US
dc.identifier.endpage397en_US
dc.identifier.issn1300-0101
dc.identifier.issn1300-0101en_US
dc.identifier.issue2en_US
dc.identifier.scopusqualityQ3en_US
dc.identifier.startpage391en_US
dc.identifier.urihttps://hdl.handle.net/11454/23414
dc.identifier.volume23en_US
dc.indekslendigikaynakScopusen_US
dc.language.isoenen_US
dc.relation.ispartofTurkish Journal of Physicsen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.titleThe Light and Colour Variations of MM Heren_US
dc.typeArticleen_US

Dosyalar

Koleksiyon

Scopus İndeksli Yayınlar Koleksiyonu