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October 16, 2025ASEAN Journal of Scientific and Technological Reports

W UMa-type Light-Curve Analysis V700 Cyg Binary Star

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Authors

SSSupat SairattanainTHTorik HengpiyaWMWiraporn Maithong

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Overview

Photometric observations show effective temperatures of 7692 K and 6078 K in a binary star system, indicating a detailed light curve analysis.

Key Points

  • The effective temperatures of the primary and secondary components are 7692 K and 6078 K, respectively.
  • A mass ratio (q) of 2.98 demonstrates the dynamics of the binary star system.
  • The degree of contact in this W UMa-type binary star system is determined to be 3.48%.
  • Light curves were generated using the Wilson-Devinney method for accurate analysis of the system's properties.

Cite This Study

Sairattanain et al. (2025) studied this question.

synapsesocial.com/papers/68f0ba59c50c73ebef9faa11https://doi.org/10.55164/ajstr.v28i6.259261
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