A Photometric Study of Four Recently Discovered Contact Binaries: 1SWASP J064501.21+342154.9, 1SWASP J155822.10-025604.8, 1SWASP J212808.86+151622.0 and UCAC4 436-062932
arXiv:1608.06488 · doi:10.3847/0004-6256/152/3/57
Abstract
We present new, high-quality multicolor observations of four recently discovered contact binaries: 1SWASP J064501.21+342154.9, 1SWASP J155822.10-025604.8, 1SWASP J212808.86+151622.0, and UCAC4 436-062932, and analyze their light curves to determine orbital and physical parameters using the modeling program of G. Djurašević. In the absence of spectroscopic observations, the effective temperatures of the brighter components are estimated from the color indices, and the mass ratios are determined with the q-search method. The analysis shows that all four systems are W UMa type binaries in shallow contact configurations, consisting of late-type main-sequence primaries and evolved secondaries with active surface regions (dark or bright spots) resulting from magnetic activity or ongoing transfer of thermal energy between the components. We compare the derived orbital and stellar parameters for these four variables with a large sample of previously analyzed W UMa stars and find that our results fit it well.
References in corpus (5)
- Masses and angular momenta of contact binary stars
- Period decrease in three SuperWASP eclipsing binary candidates near the short-period limit
- Photometric analysis of overcontact binaries AK Her, HI Dra, V1128 Tau and V2612 Oph
- Accretion disk in the eclipsing binary AU Mon
- Fundamental parameters of the close interacting binary HD170582 and its luminous accretion disc
Cited by in corpus (8)
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- Starspots in contact and semi-detached binary systems
- CoBiToM Project -- II: Evolution of contact binary systems close to the orbital period cut-off
- Comparative study of TESS photometry and radial velocities on six early K-type contact binaries with similar periods around 0.268 days
- YZ Phe: an active contact binary with variation of the O'Connell effect and orbital period change
- Light curve analysis of six totally eclipsing W UMa binaries
- The First Photometric and Spectroscopic Study of Contact Binary V2840 Cygni