Photometric investigation of the evolved contact binary system DN Aur

1996 ◽  
Vol 246 (2) ◽  
pp. 291-298 ◽  
Author(s):  
S. N. Goderya ◽  
K. C. Leung ◽  
E. G. Schmidt
2016 ◽  
Vol 2016 ◽  
pp. 1-6 ◽  
Author(s):  
Xiao Zhou ◽  
Sheng-Bang Qian ◽  
Jia Zhang ◽  
Lin-Jia Li ◽  
Qi-Shan Wang

The light curve of V921 Her in ultraviolet band observed by the Lunar-based Ultraviolet Telescope (LUT) is analyzed by the Wilson-Devinney code. Our solutions conclude that V921 Her is an early type marginal contact binary system with an additional close-in component. The binary system is under poor thermal contact with a temperature difference of nearly 700 K between the two components. The close-in component contributes about 19% of the total luminosity in the triple system. Combining the radial velocity study together with our photometric solutions, the mass of the primary star and secondary one is calculated to beM1=1.784  (±0.055)M⊙,M2=0.403  (±0.012)M⊙. The evolutionary scenario of V921 Her is discussed. All times of light minimum of V921 Her available in the bibliography are taken into account and theO-Ccurve is analyzed for the first time. The most probable fitting results are discussed in the paper, which also confirm the existence of a third component (P3=10.2year) around the binary system. The period of V921 Her is also undergoing a continuously rapid increase at a rate ofdP/dt=+2.79×10-7  day·year-1, which may be due to mass transfer from the less massive component to the more massive one.


2015 ◽  
Vol 2015 ◽  
pp. 1-8 ◽  
Author(s):  
M. M. Elkhateeb ◽  
M. I. Nouh ◽  
E. Elkholy ◽  
B. Korany

DK Cyg (P=0.4707) is a contact binary system that undergoes complete eclipses. All the published photoelectric data have been collected and utilized to reexamine and update the period behavior of the system. A significant period increase with rate of 12.590 × 10−11 days/cycle was calculated. New period and ephemeris have been calculated for the system. A long term photometric solution study was performed and a light curve elements were calculated. We investigated the evolutionary status of the system using theoretical evolutionary models.


2002 ◽  
Vol 187 ◽  
pp. 337-338
Author(s):  
A. Yamasaki ◽  
M. Takeda ◽  
T. Yamauchi ◽  
G. Takada ◽  
S. Hattori

AbstractVariability of the light curves of the short-period eclipsing binary system GR Tau (, almost-contact binary) is studied. It is found that GR Tau experienced both the state which is characterized by asymmetric light curves and the state characterized by symmetrical light curves.


1996 ◽  
Vol 246 (2) ◽  
pp. 229-242 ◽  
Author(s):  
E. Budding ◽  
C-H. Kim ◽  
O. Demircan ◽  
Z. Müyesseroğlu ◽  
K. Saijo ◽  
...  
Keyword(s):  

2016 ◽  
Vol 151 (6) ◽  
pp. 170 ◽  
Author(s):  
Chin-Ping Hu ◽  
Ting-Chang Yang ◽  
Yi Chou ◽  
L. Liu ◽  
S.-B. Qian ◽  
...  
Keyword(s):  
X Ray ◽  

2014 ◽  
Vol 14 (9) ◽  
pp. 1157-1165 ◽  
Author(s):  
Nian-Ping Liu ◽  
Sheng-Bang Qian ◽  
Wen-Ping Liao ◽  
Jia-Jia He ◽  
Er-Gang Zhao ◽  
...  

New Astronomy ◽  
2014 ◽  
Vol 28 ◽  
pp. 44-48 ◽  
Author(s):  
M. Tüysüz ◽  
F. Soydugan ◽  
S. Bilir ◽  
E. Soydugan ◽  
T. Şenyüz ◽  
...  

2015 ◽  
Vol 67 (3) ◽  
pp. 48 ◽  
Author(s):  
Wen-Ping Liao ◽  
Sheng-Bang Qian ◽  
Er-Gang Zhao ◽  
Lin-Jia Li

2006 ◽  
Vol 23 (3) ◽  
pp. 177-188 ◽  
Author(s):  
Jang-Hae Jeong ◽  
Chun-Hwey Kim ◽  
Yong-Sam Lee

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