First CCD photometric observation of the W-UMa eclipsing binary system 1SWASP J064501.21+342154.9
Essam, A., Mohamadien, G., Ahmed, N., Ali, G. (2013). First CCD photometric observation of the W-UMa eclipsing binary system 1SWASP J064501.21+342154.9. EKB Journal Management System, 2(2), 256-265. doi: 10.1016/j.nrjag.2013.12.001
A. Essam; Ghada F. Mohamadien; Nasser M. Ahmed; Gamal B. Ali. "First CCD photometric observation of the W-UMa eclipsing binary system 1SWASP J064501.21+342154.9". EKB Journal Management System, 2, 2, 2013, 256-265. doi: 10.1016/j.nrjag.2013.12.001
Essam, A., Mohamadien, G., Ahmed, N., Ali, G. (2013). 'First CCD photometric observation of the W-UMa eclipsing binary system 1SWASP J064501.21+342154.9', EKB Journal Management System, 2(2), pp. 256-265. doi: 10.1016/j.nrjag.2013.12.001
Essam, A., Mohamadien, G., Ahmed, N., Ali, G. First CCD photometric observation of the W-UMa eclipsing binary system 1SWASP J064501.21+342154.9. EKB Journal Management System, 2013; 2(2): 256-265. doi: 10.1016/j.nrjag.2013.12.001

First CCD photometric observation of the W-UMa eclipsing binary system 1SWASP J064501.21+342154.9

NRIAG Journal of Astronomy and Geophysics
Volume 2, Issue 2, December 2013, Pages 256-265    PDF (1.92 M)
DOI: 10.1016/j.nrjag.2013.12.001
Authors
A. Essam; Ghada F. Mohamadien; Nasser M. Ahmed; Gamal B. Ali
Abstract
New BVRI light curves of the eclipsing binary system 1SWASP J064501.21+342154.9 (J0645) have been constructed based on CCD observations that were obtained by using the 1.88-m telescope of Kottamia Astronomical Observatory (KAO), Egypt on January and February, 2013. New times of minima and new ephemeris have been determined from these light curves. Using the Binary Maker 3.0 (BM3) package, a preliminary determination of the geometric and photometric element parameters of the system J0645 is derived.
Keywords
Variable stars; Binary stars; Eclipsing binary; W-UMa binary system
Statistics
Article View: 4
PDF Download: 3