Light curve analysis of W UMa type eclipsing binaries selected from the Kepler archive
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Abstract (EN)
The W type Ursae Majoris (W UMa) type eclipsing binary systems are known as a low mass contact binary stars of spectral types F, G, or K. In this thesis, the light curves of W UMa type eclipsing binary systems with orbital periods (0.23
Author
Hatice Saraç
How to Cite
Hatice Saraç (Master Thesis). Light curve analysis of W UMa type eclipsing binaries selected from the Kepler archive, 2019, Osmaniye Korkut Ata University.
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