Paper:	Photometric Monitoring of GSC 2696-2622 Variability
Volume:	424, Proceedings of the 9th International Conference of the Hellenic Astronomical Society
Page:	212
Authors:	Nanouris, N.; Antonopoulou, E.
Abstract:	The poster deals with the possible variability of GSC 2696-2622. GSC 2696-2622 is located in the vicinity of the eclipsing binary CG Cyg and thus the former has been chosen several times as a comparison star of the latter. Therefore, variability in the brightness of GSC 2696-2622 could lead to incorrect conclusions of the CG Cyg behavior, a fact that renders the clarification of its photometric features highly crucial. Our work focuses on high resolution and precision photometric observations taken by two observatories during July of 2008. The results, supported by Fourier analysis, confirm that the star is a semi-periodic one with variable amplitude that varies on hourly timescales.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.066 seconds