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Radial Velocity and Light Curves Analysis of the Contact Binary V1073 Cygni
Authors:M. Jafari  B. Khalesseh  R. Pazhouhesh
Affiliation:(1) School of Physics, Damghan University of Basic Sciences, Damghan, Iran;(2) Physics Department, School of Sciences, Ferdowsi University, Mashhad, Iran;(3) Physics Department, School of Sciences, Birjand University, Birjand, Iran
Abstract:In this study complete BV light curves of the W Ursae Majoris binary V1073 Cygni obtained in 2005 are presented. We have used the spectroscopic data of V1073 Cyg obtained by Ahn et al. (1992) for analysis. The analysis of radial velocity and light curves was made with Wilson} program (1998) and the geometric and physical elements} of the system were derived. By searching the simultaneous} solutions of the system, we have determined the masses and radii of the components: 1.64M, 2.275R for the primary component and 0.55M, 1.397R for the secondary component respectively. The effective temperature of 6494 ± 53 K for the secondary component was also estimated.
Keywords:Stars  Variable  Binaries  Eclipsing binary  Individual  V1073 Cygni
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