Please use this identifier to cite or link to this item: https://hdl.handle.net/11147/5363
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dc.contributor.authorUlusoy, Ceren-
dc.contributor.authorGülmez, T.-
dc.contributor.authorStateva, I.-
dc.contributor.authorDimitrov, D.-
dc.contributor.authorIliev, I. Kh.-
dc.contributor.authorKobulnicky, H. A.-
dc.contributor.authorYaşarsoy, B.-
dc.contributor.authorAlvarez, M.-
dc.contributor.authorMichel, R.-
dc.contributor.authorFox Machado, L.-
dc.contributor.authorDamasso, M.-
dc.contributor.authorCarbognani, A.-
dc.contributor.authorCenadelli, D.-
dc.contributor.authorPickering, T. E.-
dc.contributor.authorKwon, J.-
dc.contributor.authorTamura, M.-
dc.contributor.authorBalona, L. A.-
dc.date.accessioned2017-04-20T10:48:57Z-
dc.date.available2017-04-20T10:48:57Z-
dc.date.issued2013-
dc.identifier.citationUlusoy, C., Gülmez, T., Stateva, I., Dimitrov, D., Iliev, I. Kh., Kobulnicky, H. A., Yaşarsoy, B., ...Balona, L. A. (2013). Mode identification in the high-amplitude δ Scuti star V2367 Cyg. Monthly Notices of the Royal Astronomical Society, 428(4), 3551-3558. doi:10.1093/mnras/sts293en_US
dc.identifier.issn1365-2966-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://doi.org/10.1093/mnras/sts293-
dc.identifier.urihttp://hdl.handle.net/11147/5363-
dc.description.abstractWe report on a multisite photometric campaign on the high-amplitude delta Scuti star V2367 Cyg in order to determine the pulsation modes. We also used high-dispersion spectroscopy to estimate the stellar parameters and projected rotational velocity. Time series multicolour photometry was obtained during a 98-d interval from five different sites. These data were used together with model atmospheres and non-adiabatic pulsation models to identify the spherical harmonic degree of the three independent frequencies of highest amplitude as well as the first two harmonics of the dominant mode. This was accomplished by matching the observed relative light amplitudes and phases in different wavebands with those computed by the models. In general, our results support the assumed mode identifications in a previous analysis of Kepler data. © 2012 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.en_US
dc.description.sponsorshipSouth African National Research Foundation; NRF; Bulgarian NSF; South African Astronomical Observatory; UNAM; CONACyT; European Union; Autonomous Region of the Aosta Valley; Italian Department for Work, Health and Pensions; Regional Government of the Aosta Valley; Town Municipality of Nus; Mont Emilius Community; National Research Foundation of South Africaen_US
dc.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectV2367 Cygen_US
dc.subjectStarsen_US
dc.subjectDelta Scutien_US
dc.subjectOscillationsen_US
dc.subjectIndividualen_US
dc.titleMode identification in the high-amplitude {\delta} Scuti star V2367 Cygen_US
dc.typeArticleen_US
dc.institutionauthorUlusoy, Ceren-
dc.departmentIzmir Institute of Technology. Physicsen_US
dc.identifier.volume428en_US
dc.identifier.issue4en_US
dc.identifier.startpage3551en_US
dc.identifier.endpage3558en_US
dc.identifier.wosWOS:000318232000057en_US
dc.identifier.scopus2-s2.0-84873727305en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.identifier.doi10.1093/mnras/sts293-
dc.relation.doi10.1093/mnras/sts293en_US
dc.coverage.doi10.1093/mnras/sts293en_US
dc.identifier.scopusqualityQ1-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.fulltextWith Fulltext-
item.grantfulltextopen-
item.openairetypeArticle-
item.languageiso639-1en-
Appears in Collections:Physics / Fizik
Scopus İndeksli Yayınlar Koleksiyonu / Scopus Indexed Publications Collection
WoS İndeksli Yayınlar Koleksiyonu / WoS Indexed Publications Collection
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