The chromospherically--active binary CF Tuc revisited
D. Dogru, A. Erdem, S. S. Dogru, S. Zola

TL;DR
This study provides updated orbital and physical parameters of the active binary CF Tuc using new spectra, light curves, and advanced analysis methods, revealing complex period variations possibly due to a third body or magnetic activity.
Contribution
The paper presents new high-resolution spectroscopic data and refined orbital parameters for CF Tuc, incorporating light curve analysis and period variation studies, including potential evidence for a third body.
Findings
New radial velocity curves and orbital elements obtained.
Detection of Hα and CaII emissions indicating chromospheric activity.
Possible presence of a third body affecting orbital period variations.
Abstract
New high-resolution spectra, of the chromospherically active binary system CF Tuc, taken at the Mt. John University Observatory in 2007, were analyzed using two methods: cross-correlation and Fourier--based disentangling. As a result, new radial velocity curves of both components were obtained. The resulting orbital elements of CF Tuc are: = AU, = AU, = , and = . The cooler component of the system shows H and CaII H & K emissions. Our spectroscopic data and recent light curves were solved simultaneously using the Wilson-Devinney code. A dark spot on the surface of the cooler component was assumed to explain large asymmetries observed in the light curves. The following absolute parameters of the components were determined:…
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