A Photometric Analysis of Az Vir
We present photometric analysis of the eclipsing binary star system Az Vir. The light curves presented are produced using data collected using the 17-inch PlaneWave telescope at the Truman State University Observatory utilizing Johnson B, Johnson V, and Johnson R filters. We collected additional data using the 31-inch NURO telescope at the Lowell Observatory complex in Flagstaff, AZ using Bessel B, Bessel V, and Bessel R filters. We use these data to generate light curves and then apply an 8-term truncated Fourier fit in order to confirm the classification of Az Vir as a W Ursae Majoris-type eclipsing variable. In addition, we use data provided by the SuperWASP mission to perform a long term O-C (observed minus calculated) analysis on the system to determine if and how the period is changing.
Keywords: eclipsing, binary, Photometry, Lowell, NURO, Observatory, SuperWASP, Fourier
Topic(s):Physics-Astronomy
Astronomy
Physics
Presentation Type: Oral Paper
Session: 306-4
Location: MG 2050
Time: 1:45