scholarly journals New Photometric Elements of the Eclipsing Binary X Trianguli

1973 ◽  
Vol 85 ◽  
pp. 112
Author(s):  
J. Scott Shaw ◽  
Karen L. Kusler
1986 ◽  
Vol 125 (1) ◽  
pp. 181-188 ◽  
Author(s):  
J. M. Garc�a ◽  
A. Gim�nez

1983 ◽  
Vol 304 (5) ◽  
pp. 263-264
Author(s):  
G. Giuricin ◽  
F. Mardirossian ◽  
M. Mezzetti

1980 ◽  
Vol 73 (2) ◽  
pp. 389-394 ◽  
Author(s):  
G. Giuricin ◽  
F. Mardirossian ◽  
F. Predolin

2011 ◽  
Vol 55 (11) ◽  
pp. 989-999 ◽  
Author(s):  
M. V. Kuznetsov ◽  
Kh. F. Khaliullin ◽  
A. I. Khaliullina ◽  
V. G. Metlov ◽  
L. V. Mossakovskaya

2005 ◽  
Vol 31 (2) ◽  
pp. 117-128 ◽  
Author(s):  
V. S. Kozyreva ◽  
A. V. Kusakin ◽  
Kh. F. Khaliullin

2011 ◽  
Vol 7 (S282) ◽  
pp. 55-56
Author(s):  
Alexios Liakos ◽  
Panagiotis Niarchos ◽  
Edwin Budding

AbstractCCD photometric observations of the Algol-type eclipsing binary AT Peg have been obtained. The light curves are analyzed with modern techniques and new geometric and photometric elements are derived. A new orbital period analysis of the system, based on the most reliable timings of minima found in the literature, is presented and apparent period modulations are discussed with respect to the Light-Time effect (LITE) and secular changes in the system. The results of these analyses are compared and interpreted in order to obtain a coherent view of the system's behaviour.


1998 ◽  
Vol 11 (1) ◽  
pp. 394-394
Author(s):  
Adbdulrahman Ali S. Malawi

New CCD observations of the eclipsing binary VW Cephei were made on the 9th and 10th of October 1996 and on the 11th of Nov. 1996. The light curves and short time-scale variations are discussed. Photometric elements were determined from analyses of the light curves. These new solutions are also discussed.


2013 ◽  
Vol 9 (S301) ◽  
pp. 507-508 ◽  
Author(s):  
Burak Ulaş ◽  
Ceren Ulusoy ◽  
Kosmas Gazeas ◽  
Naci Erkan ◽  
Alexios Liakos

AbstractWe present new photometric observations of two eclipsing binary systems, V1241 Tau and GQ Dra. We use the following methodology: initially, the Wilson-Devinney code is applied to the light curves in order to determine the photometric elements of the systems. Then, the residuals are analysed using Fourier techniques. The results are the following. One frequency can be possibly attributed to a real light variation of V1241 Tau, while there is no evidence of pulsations in the light curve of GQ Dra.


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