scholarly journals Hi-fi phenomenological description of eclipsing binary light variations as the basis for their period analysis

2013 ◽  
Vol 64 ◽  
pp. 299-302 ◽  
Author(s):  
Z. Mikulášek ◽  
M. Zejda ◽  
M. Chrastina ◽  
S.-B. Qian ◽  
L.-Y. Zhu
Keyword(s):  
Phenomenological Description ◽  
Period Analysis ◽  
Eclipsing Binary

Period analysis of the eclipsing binary AI Dra

2009 ◽  
Vol 326 (1) ◽  
pp. 119-123 ◽  
Author(s):  
P. Zasche ◽  
R. Uhlář ◽  
P. Svoboda
Keyword(s):  
Period Analysis ◽  
Eclipsing Binary

First orbital period analysis of the Algol-type eclipsing binary RZ Aurigae

New Astronomy ◽  
2010 ◽  
Vol 15 (4) ◽  
pp. 392-395 ◽  
Author(s):  
Y.-G. Yang ◽  
H.-F. Dai ◽  
X.-G. Yin
Keyword(s):  
Orbital Period ◽  
Period Analysis ◽  
Eclipsing Binary

scholarly journals Light Curve and Orbital Period Analysis of the Eclipsing Binary AT Peg

2011 ◽  
Vol 7 (S282) ◽  
pp. 55-56
Author(s):  
Alexios Liakos ◽  
Panagiotis Niarchos ◽  
Edwin Budding
Keyword(s):  
Light Curve ◽  
Orbital Period ◽  
Time Effect ◽  
Light Curves ◽  
Period Analysis ◽  
Eclipsing Binary ◽  
Secular Changes ◽  
Photometric Observations ◽  
Photometric Elements

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.

Updated UBV Light-Curve and Period Analysis of Eclipsing Binary HS Herculis

2006 ◽  
Vol 304 (1-4) ◽  
pp. 29-33 ◽  
Author(s):  
Zeynep Bozkurt ◽  
Ömer Lütfi Değirmenci
Keyword(s):  
Light Curve ◽  
Period Analysis ◽  
Eclipsing Binary

The first BVR light curves and period analysis of the eclipsing binary V821 Cas

New Astronomy ◽  
2007 ◽  
Vol 12 (4) ◽  
pp. 322-326 ◽  
Author(s):  
O DEGIRMENCI ◽  
Z BOZKURT ◽  
K YAKUT ◽  
O DEMIRCAN ◽  
A ERDEM ◽  
...  
Keyword(s):  
Light Curves ◽  
Period Analysis ◽  
Eclipsing Binary

Solution of basic tasks in eclipsing binary period analysis by genetic and LSM algorithms

2013 ◽  
Vol 64 ◽  
pp. 383-384 ◽  
Author(s):  
M. Chrastina ◽  
Z. Mikulášek ◽  
M. Zejda
Keyword(s):  
Period Analysis ◽  
Eclipsing Binary

The Eclipsing Binary WX Eridani

1979 ◽  
Vol 46 ◽  
pp. 385
Author(s):  
M.B.K. Sarma ◽  
K.D. Abhankar
Keyword(s):  
Light Curve ◽  
Spectral Type ◽  
Orbital Period ◽  
Primary Component ◽  
Light Curves ◽  
Absorption Feature ◽  
Primary Star ◽  
Eclipsing Binary ◽  
The Times ◽  
Phase Angles

AbstractThe Algol-type eclipsing binary WX Eridani was observed on 21 nights on the 48-inch telescope of the Japal-Rangapur Observatory during 1973-75 in B and V colours. An improved period of P = 0.82327038 days was obtained from the analysis of the times of five primary minima. An absorption feature between phase angles 50-80, 100-130, 230-260 and 280-310 was present in the light curves. The analysis of the light curves indicated the eclipses to be grazing with primary to be transit and secondary, an occultation. Elements derived from the solution of the light curve using Russel-Merrill method are given. From comparison of the fractional radii with Roche lobes, it is concluded that none of the components have filled their respective lobes but the primary star seems to be evolving. The spectral type of the primary component was estimated to be F3 and is found to be pulsating with two periods equal to one-fifth and one-sixth of the orbital period.

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