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astro-ph.SR2026★ 3 cited
Detailed Investigation of a W UMa Contact Binary with an Ultralow Mass Ratio and a Third-Body as a Potential Merger Candidate
Atila Poro, Ehsan Paki, Fahri Alicavus +1
The lower limit of the mass ratio in contact binaries remains uncertain, with observations suggesting systems exist below theoretical predictions. The stability of such very low ma…
astro-ph.SR2025
The BSN Application-I: Photometric Light Curve Solutions of Contact Binary Systems
Ehsan Paki, Atila Poro, Minoo Dokht Moosavi Rowzati
Light curve analysis of W UMa-type contact binary systems using MCMC or MC methods can be time-consuming, primarily because the repeated generation of synthetic light curves tends…
astro-ph.SR2024
Reanalyzing the Light Curves and Absolute Parameters of Twenty Contact Binary Stars Using TESS Data
Ehsan Paki, Atila Poro
Reanalyzing contact binaries with space-based photometric data and investigating possible parameter changes can yield accurate samples for theoretical studies. We investigated ligh…