Light Curve Analysis Of W-uma Type Binary Systems Rz Umi, Oq Uma, Lp Uma
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arXiv
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| Format: | Preprint |
| Published: |
2025
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| _version_ | 1866911031923572736 |
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| author | Grozdanović, Marko Đurašević, Gojko |
| author_facet | Grozdanović, Marko Đurašević, Gojko |
| contents | This study presents new, high-quality, optical photometric observations of three W UMa type contact binaries. The analysis of the corresponding light curves is made using Djurasevic's inverse problem method. To explain the light curve asymmetries and variations, we used the Roche model that involved regions containing spots on the components. The fundamental parameters of these systems were derived, including the mass ratios determined using the q-search method. Hypotheses involving active surface regions, such as dark spots on the primary and secondary components, or bright spots in the neck region due to magnetic activity or continuous mass transfer between components, were examined to explain the varying amplitudes of maxima and nearly equal minima depths in the light curves. Using the derived orbital and physical parameters, three-dimensional models were constructed for various orbital phases. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2507_00768 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Light Curve Analysis Of W-uma Type Binary Systems Rz Umi, Oq Uma, Lp Uma Grozdanović, Marko Đurašević, Gojko Solar and Stellar Astrophysics This study presents new, high-quality, optical photometric observations of three W UMa type contact binaries. The analysis of the corresponding light curves is made using Djurasevic's inverse problem method. To explain the light curve asymmetries and variations, we used the Roche model that involved regions containing spots on the components. The fundamental parameters of these systems were derived, including the mass ratios determined using the q-search method. Hypotheses involving active surface regions, such as dark spots on the primary and secondary components, or bright spots in the neck region due to magnetic activity or continuous mass transfer between components, were examined to explain the varying amplitudes of maxima and nearly equal minima depths in the light curves. Using the derived orbital and physical parameters, three-dimensional models were constructed for various orbital phases. |
| title | Light Curve Analysis Of W-uma Type Binary Systems Rz Umi, Oq Uma, Lp Uma |
| topic | Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2507.00768 |