SIMBAD references

2015AJ....149..197Z - Astron. J., 149, 197 (2015/June-0)

Ten Kepler eclipsing binaries containing the third components.

ZASCHE P., WOLF M., KUCAKOVA H., VRASTIL J., JURYSEK J., MASEK M. and JELINEK M.

Abstract (from CDS):

Analyzing the available photometry from the Kepler satellite and other databases, we performed detailed light curve modeling of 10 eclipsing binary systems that were found to exhibit a periodic modulation of their orbital periods. All of the selected systems are detached Algol type, with orbital periods from 0.9 to 2.9 days. In total, 9448 times of minimum for these binaries were analyzed in an attempt to identify the period variations caused by the third bodies in these systems. The well-known method of the light-travel time effect was used for the analysis. The orbital periods of the outer bodies were found to be between 1 and 14 years. This hypothesis makes such systems interesting for future prospective detections of these components, despite their low predicted masses. Considering the dynamical interaction between the orbits, the system KIC 3440230 seems to be the most interesting, in which one would expect the detection of some effects (i.e., changing the inclination) even after a few years or decades of observations.

Abstract Copyright:

Journal keyword(s): binaries: eclipsing - stars: fundamental parameters - stars: individual: (KIC 2305372, KIC 3440230, KIC 5513861, KIC 5621294, KIC 7630658, KIC 8553788, KIC 9007918, KIC 9402652, KIC 10581918, KIC 10686876)

VizieR on-line data: <Available at CDS (J/AJ/149/197): table1.dat table3.dat table5.dat refs.dat>

Simbad objects: 22

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2020.09.28-18:40:56

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