Publication:
Analysis of the Light Curves of PV Cassiopeiae by Use of Automatized Fourier Techniques

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dc.contributor.authorAlkan H.
dc.date.accessioned2020-06-21T09:20:42Z
dc.date.available2020-06-21T09:20:42Z
dc.date.issued1981
dc.departmentOMÜen_US
dc.department-tempAlkan, H., Faculty of Science and Engineering, Ondokuzmayis University, Samsun, Turkey --en_US
dc.description.abstractUBV Light Curves of the eclipsing binary system PV Cassiopeiae have been investigated using recently developed frequency-domain techniques. This analysis is based on Kopal's new theory for the study of the light variations, between minima as well as within eclipses, of eclipsing binaries whose components undistorted or distorted by axial rotation and mutual tidal action. A method for the distinguishing of the photometric proximity and eclipse effects directly from the observed data is also presented. In this method no 'rectification' is needed. The automated method has been tested successfully on the light curves of PV Cassiopeiae. Finally, a comparative discussion is given of Kopal's and Kitamura's methods of the light curves analysis. © 1981 D. Reidel Publishing Co.en_US
dc.identifier.doi10.1007/BF00648655
dc.identifier.endpage463en_US
dc.identifier.issn0004-640X
dc.identifier.issue2en_US
dc.identifier.startpage455en_US
dc.identifier.urihttps://doi.org/10.1007/BF00648655
dc.identifier.urihttps://hdl.handle.net/20.500.12712/3352
dc.identifier.volume75en_US
dc.language.isoenen_US
dc.publisherKluwer Academic Publishersen_US
dc.relation.journalAstrophysics and Space Scienceen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.titleAnalysis of the Light Curves of PV Cassiopeiae by Use of Automatized Fourier Techniquesen_US
dc.typeArticleen_US
dspace.entity.typePublication

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