THE CHALLENGES OF MODELLING THE ACTIVITIES OCCURRING ON ECLIPSING BINARIES V1130 CYG AND V461 LYR

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dc.authoridYoldas, Ezgi/0000-0003-2017-3796
dc.authorscopusid57188930042
dc.authorscopusid22033975800
dc.contributor.authorYoldas, E.
dc.contributor.authorDal, H. A.
dc.date.accessioned2023-01-12T20:11:52Z
dc.date.available2023-01-12T20:11:52Z
dc.date.issued2021
dc.departmentN/A/Departmenten_US
dc.description.abstractWe present the findings for the magnetic activities seen on V1130 Cyg and V461 Lyr. In the case of V1130 Cyg, the secondary component's temperature was found to be 3891 +/- 50 K, while the mass ratio was computed as 0.689 +/- 0.001, and the orbital inclination as 90 degrees.00 +/- 0 degrees.01. The temperature of V461 Lyr's secondary component was found to be 4206 +/- 50 K, and the mass ratio was calculated as 0.999 +/- 0.001 with 89 degrees.58 +/- 0 degrees.01 of orbital inclination. The analyses exhibit the effects of the stellar spots on the light curves. The models indicate that there are two types of flares in the case of V1130 Cyg, and three types of flares for V461 Lyr. The Plateau parameters have been found as 2.1997 s for Group 1 and 1.0068 s for Group 2 in the case of V1130 Lyr. They have been computed as 1.9015 s for Group 1, 2.7943 s for Group 2, and 3.4324 s for Group 3 of V461 Lyr.en_US
dc.description.sponsorshipTurkish Scientific and Tech-nical Research Council (TdUBITAK) [116F213]en_US
dc.description.sponsorshipWe thank the referee for useful comments that contributed to the improvement of the paper. We also wish to thank the Turkish Scientific and Tech-nical Research Council (TdUBITAK) for supporting this work through Grant No. 116F213.en_US
dc.identifier.doi10.22201/ia.01851101p.2021.57.02.07
dc.identifier.endpage349en_US
dc.identifier.issn0185-1101
dc.identifier.issn0185-1101en_US
dc.identifier.issue2en_US
dc.identifier.scopus2-s2.0-85118477301en_US
dc.identifier.scopusqualityQ3en_US
dc.identifier.startpage335en_US
dc.identifier.urihttps://doi.org/10.22201/ia.01851101p.2021.57.02.07
dc.identifier.urihttps://hdl.handle.net/11454/78206
dc.identifier.volume57en_US
dc.identifier.wosWOS:000782660100007en_US
dc.identifier.wosqualityQ4en_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.language.isoenen_US
dc.publisherUniv Nacional Autonoma Mexico, Inst De Astronomiaen_US
dc.relation.ispartofRevista Mexicana De Astronomia Y Astrofisicaen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectmethods: data analysisen_US
dc.subjectstars: binaries: eclipsingen_US
dc.subjectstars: flareen_US
dc.subjectstars: individual: V1130 Cyg, V461 Lyren_US
dc.subjecttechniques: photometricen_US
dc.subjectWhite-Light Flaresen_US
dc.subjectChromospheric Variationsen_US
dc.subjectKepleren_US
dc.subjectStarsen_US
dc.subjectEnergeticsen_US
dc.subjectEvolutionen_US
dc.subjectCurvesen_US
dc.subjectIi.en_US
dc.titleTHE CHALLENGES OF MODELLING THE ACTIVITIES OCCURRING ON ECLIPSING BINARIES V1130 CYG AND V461 LYRen_US
dc.typeArticleen_US

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