The Photometric Study of Six W UMa Systems and Investigation of the Mass–Radius Relations for Contact Binary Stars [PDF]
Publications of the Astronomical Society of the Pacific, 2022 We present the photometric analysis of six short-period systems (EI Oct, V336 TrA, NX Boo, V356 Boo, PS Boo, and V2282 Cyg). This is the first photometric analysis of these systems except for V336 TrA.
Atila Poro +15 more
semanticscholar +4 more sources
The Astrophysical Journal, 1981 Densities, corrected primary colors, minimum periods, inferred masses, luminosities, and specific angular momenta are computed from data on 37 W Ursae Majoris systems. A-type systems, having lower densities and angular momenta than the W-type systems, are shown to be evolved, and a new class of contact binary is identified, the OO Aquilae systems ...
S. Mochnacki
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BSN. V. The First Detailed Light Curve Modeling of Eight Totally Eclipsing Contact Binary Stars Using Ground-based and TESS Observations [PDF]
Publications of the Astronomical Society of the PacificThis study broadens our comprehensive investigation of total-eclipse W Ursae Majoris-type contact binaries by analyzing eight additional systems, continuing our previous research.
Atila Poro +5 more
semanticscholar +4 more sources
BSN-III: The First Multiband Photometric Study on the Eight Total Eclipse Contact Binary Stars [PDF]
This study continues our in-depth investigation of total-eclipse W Ursae Majoris-type contact binaries by analyzing eight new systems, complementing our previous work.
Atila Poro +8 more
semanticscholar +3 more sources
The Short Period End of the Distribution of Contact Binary Stars [PDF]
, 2013 Presented at the "40 Years of Variable Stars: A Celebration of Contributions by Horace A. Smith" conference (arXiv:1310.0149).
Lawrence A. Molnar +2 more
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Binary Analysis and Period Study of the Long-period, High-mass-ratio Contact Binary KIC 7766185
The Astronomical JournalWe present an in-depth photometric and spectroscopic study of the contact binary KIC 7766185. Spectroscopic observations were conducted on the Mayall 4 m telescope at Kitt Peak National Observatory and used to extract radial velocities.
Conor M. Larsen, Andrej Prša
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BSN. II. The First Light Curve Study of Eight Total Eclipsing Contact Binary Stars with Shallow Fillout Factors [PDF]
Astronomical JournalThis study provides the first comprehensive analysis of eight total-eclipse W Ursae Majoris-type contact binary systems. Ground-based photometric multiband observations were conducted at a Mexican observatory, and new times of minima were extracted.
Atila Poro +8 more
semanticscholar +4 more sources
On the maintenance of a temperature discontinuity in contact binary stars [PDF]
Monthly Notices of the Royal Astronomical Society, 1979 J. C. B. Papaloizou, J. E. Pringle
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Models of Close and Contact Binary Stars--I: Polytropic Models [PDF]
Monthly Notices of the Royal Astronomical Society, 1970 B. R. Durney, I. W. Roxburgh
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The uniqueness of determination of the photometric mass ratio of contact binary stars with applications to selected binaries [PDF]
Contributions of the Astronomical Observatory Skalnaté Pleso. We have used a Roche-geometry code to pre-generate light curves of contact binary stars using only mass ratio q , fill out f of the Roche lobes, and the inclination i of the orbital plane.
Ľ. Hambálek, T. Pribulla
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