Analysis of light curve and orbital period of contact binary NO Vul

dc.contributor.authorYıldırım, Muhammed Faruk
dc.contributor.authorSoydugan, Faruk
dc.date.accessioned2025-01-27T19:26:47Z
dc.date.available2025-01-27T19:26:47Z
dc.date.issued2021
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractIn this study, we investigated light curve analysis of contact binary system NO Vul. Also, we investigated orbital period variations of contact binaries NO Vul based on all published minima times and also those obtained from our own observations. Photometric observations are obtained from the ASAS public archive. Physical parameters of the system are derived using the modeling code by Wilson and Dewinney’s (WD). Photometric results indicate that NO Vul is q = 0.72(2) and about f =%19 respectively and the derived orbital inclination i =77(1).
dc.identifier.doi10.25092/baunfbed.826104
dc.identifier.endpage38
dc.identifier.issn1301-7985
dc.identifier.issn2536-5142
dc.identifier.issue1
dc.identifier.startpage30
dc.identifier.trdizinid432142
dc.identifier.urihttps://doi.org/10.25092/baunfbed.826104
dc.identifier.urihttps://search.trdizin.gov.tr/tr/yayin/detay/432142
dc.identifier.urihttps://hdl.handle.net/20.500.12428/15626
dc.identifier.volume23
dc.indekslendigikaynakTR-Dizin
dc.language.isoen
dc.relation.ispartofBalıkesir Üniversitesi Fen Bilimleri Enstitüsü Dergisi
dc.relation.publicationcategoryMakale - Ulusal Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_TRD_20250125
dc.subjectMatematik
dc.subjectFizik
dc.subjectMatematik
dc.subjectAstronomi ve Astrofizik
dc.titleAnalysis of light curve and orbital period of contact binary NO Vul
dc.typeArticle

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