scholarly journals Correction to: Light Curve Analysis of some Eclipsing Binary Systems

Astrophysics ◽  
2021 ◽  
Vol 64 (3) ◽  
pp. 425-425
Author(s):  
M. S. Alenazi ◽  
M. M. Elkateeb
Keyword(s):  
Light Curve ◽  
Binary Systems ◽  
Curve Analysis ◽  
Light Curve Analysis ◽  
Eclipsing Binary

scholarly journals Light curve analysis of the eclipsing binary system V781 Tau

2021 ◽  
Vol 2145 (1) ◽  
pp. 012005
Author(s):  
N Lamlert ◽  
W Maithong
Keyword(s):  
Binary System ◽  
Light Curve ◽  
Orbital Period ◽  
Binary Systems ◽  
Curve Analysis ◽  
Photometric System ◽  
Light Curve Analysis ◽  
Eclipsing Binary ◽  
The Public ◽  
Secondary Star

Abstract V781 Tau is one of W UMa eclipsing binary systems whose orbital period is 0.34 days. The 0.7-meter telescope with CCD photometric system in B and V filters was conducted at the Regional Observatory for the Public, Chachoengsao, Thailand during December 2018, UT. The Wilson-Devinney Technique was used for calculating the physical properties of V781 Tau. The results showed the inclination of their orbital is 66.140°±0.14. The effective temperature of the primary and secondary star is 6,060 and 5,881 K, respectively and the degree of contact is 4.38 %

Light Curve Analysis of some Eclipsing Binary Systems

Astrophysics ◽  
2021 ◽  
Vol 64 (1) ◽  
pp. 33-40
Author(s):  
M. S. Aleanzi ◽  
M. M. Elkateeb
Keyword(s):  
Light Curve ◽  
Binary Systems ◽  
Curve Analysis ◽  
Light Curve Analysis ◽  
Eclipsing Binary

Light Curve Analysis and Evolutionary Status of the RS CVn type Eclipsing Binary RZ Eridani

Algols ◽  
1989 ◽  
pp. 357-357
Author(s):  
P. Vivekananda Rao ◽  
B. V. N. S. Prakash Rao ◽  
M. B. K. Sarma
Keyword(s):  
Light Curve ◽  
Curve Analysis ◽  
Evolutionary Status ◽  
Light Curve Analysis ◽  
Eclipsing Binary

Photometric study and light curve analysis of eclipsing binary V2480 Cyg

New Astronomy ◽  
2017 ◽  
Vol 53 ◽  
pp. 1-5
Author(s):  
H. Shamsollahi ◽  
A. Jahan ◽  
R. Heidarnia
Keyword(s):  
Light Curve ◽  
Curve Analysis ◽  
Photometric Study ◽  
Light Curve Analysis ◽  
Eclipsing Binary

First ground-based photometry and light-curve analysis of the eccentric eclipsing binary V744 Cas

2006 ◽  
Vol 327 (9) ◽  
pp. 912-916 ◽  
Author(s):  
İ. Bulut ◽  
C. Çiçek ◽  
A. Erdem ◽  
V. Bakis ◽  
O. Demircan ◽  
...  
Keyword(s):  
Light Curve ◽  
Curve Analysis ◽  
Light Curve Analysis ◽  
Eclipsing Binary

scholarly journals Light curve analysis of Hipparcos data for the massive O-type eclipsing binary UW CMa

New Astronomy ◽  
2011 ◽  
Vol 16 (3) ◽  
pp. 177-182 ◽  
Author(s):  
E.A. Antokhina ◽  
M. Srinivasa Rao ◽  
M. Parthasarathy
Keyword(s):  
Light Curve ◽  
Curve Analysis ◽  
Light Curve Analysis ◽  
Eclipsing Binary

scholarly journals Synthetic Light Curve Analysis of the Close Binary Systems BX Andromedae and RR Leporis

1989 ◽  
Vol 107 ◽  
pp. 359-360
Author(s):  
R.G. Samec ◽  
R.E. Fuller ◽  
R. H. Kaitchuck ◽  
B. B. Bookmyer ◽  
D. R. Faulkner
Keyword(s):  
Light Curve ◽  
Binary Systems ◽  
Thermal Relaxation ◽  
Curve Analysis ◽  
Light Curves ◽  
Close Binary ◽  
Comparison Star ◽  
Short Time Scale ◽  
Light Curve Analysis ◽  
Short Period

AbstractUnpublished photoelectric observations of the systems BX And and RR Lep were subjected to light curve analysis using the Wilson-Devinney Code.The short-period eclipsing binary system BX And was observed on five nights in 1976 at the Morgan-Monroe station of the Goethe Link Observatory of Indiana University. The observations covering the eclipse portions of the light curves yielded four times of minimum light. A period study covering 89 years of observations confirms that a major period change took place about 1950. The system is suspected of being quite active on a short time scale. Standard magnitudes were derived for BX And and for the comparison star. The corrected color indices indicate that BX And and the comparison star BD+39° 476 are in the spectral range of F3-F5. The light curves, defined by 1092 observations in B, 1097 in V and 971 in the U filter are symmetric. The difference in the eclipse depths are quite large averaging 0.m46. A distinct de-reddening of the light curves occurs during the secondary eclipse. The first synthetic light curve solutions of the system were obtained. The solution of BX And indicates that the system consists of an F-type primary and a K-type secondary component in a state of shallow contact. This result is supported by the location of BX And on the Eggen period-color diagram for contact binaries. The large mass ratio, temperature disparity and period increase are found to be consistent with an early contact phase of thermal relaxation oscillations.

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