New Ccd Photometric Observations Of W-Uma Eclipsing Binary Nsv 5904 Using The 1.88-M Kottamia Telescope, Egypt
A Essam, A Naklawy, AA Haroon, MA Hamdy… - arXiv preprint arXiv …, 2012 - arxiv.org
arXiv preprint arXiv:1211.1329, 2012•arxiv.org
New BVR light curves of the eclipsing binary system NSV 5904 have been constructed
based on CCD observations obtained using 1.88-m telescope of Kottamia observatory
during the phase of telescope testing and adjusting its optical quality on May, 2009. New
times of minima and epoch have been determined from these light curves. Using the Binary
Maker 3.0 (BM3) package, a preliminary determination of the photometric orbital and
physical parameters of NSV 5904 are given.
based on CCD observations obtained using 1.88-m telescope of Kottamia observatory
during the phase of telescope testing and adjusting its optical quality on May, 2009. New
times of minima and epoch have been determined from these light curves. Using the Binary
Maker 3.0 (BM3) package, a preliminary determination of the photometric orbital and
physical parameters of NSV 5904 are given.
New BVR light curves of the eclipsing binary system NSV 5904 have been constructed based on CCD observations obtained using 1.88-m telescope of Kottamia observatory during the phase of telescope testing and adjusting its optical quality on May, 2009. New times of minima and epoch have been determined from these light curves. Using the Binary Maker 3.0 (BM3) package, a preliminary determination of the photometric orbital and physical parameters of NSV 5904 are given.
arxiv.org