| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 5487789 | New Astronomy | 2017 | 4 Pages |
Abstract
We present the first light curve analysis and modeling for the short period close binary 1SWASP J222514.69â+â361643.0. The results show that the system is in over contact with factor ÆÂ =â53%. The primary component is the massive and hotter one. The system is A-subtype W UMa eclipsing binary with spectral types K2 and K3, respectively.
Keywords
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
M.H. El-Depsey, M.S. Abo-Alazm, M.S. Saad, I.A. Hassan, A.M.K. Shaltout, I. Zeid, A. Shokry, M. Darwish,