| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 5487800 | New Astronomy | 2017 | 5 Pages |
Abstract
We present the photometric analysis of the detached eclipsing binary V2480 Cyg. After taking the photometric data, the light curve was analyzed in PHOEBE software, which uses the Wilson-Devinney code. Due to the observed O'Connell (1951) effect in light curve, we introduce a spotted model with 3 spots on the components, and the exact parameters of the system have been achieved. The main parameters of the system were calculated as about qptm = 1.7, Teff1 = 8075°K and Teff2 = 3829°K.
Related Topics
Physical Sciences and Engineering
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Astronomy and Astrophysics
Authors
H. Shamsollahi, A. Jahan, R. Heidarnia,