The Triply Eclipsing Hierarchical Triple Star KIC002856960
arXiv:1211.2262 · doi:10.1088/0004-637X/763/2/74
Abstract
In a recent study, Armstrong et al. presented an eclipsing binary star of about 6.2 h period with transit-like tertiary signals occurring every 204.2 d in the {\it Kepler} public data of KIC002856960 and proposed three possible hierarchical structures: (AB)b, (AB)C, and A(BC). We analyzed the {\it Kepler} light curve by including a third light source and one starspot on each binary component. The results represent that the close eclipsing pair is in a low-mass eccentric-orbit, detached configuration. Based on 123 eclipse timings calculated from the Wilson-Devinney binary model, a period study of the close binary reveals that the orbital period has experienced a sinusoidal variation with a period and a semi-amplitude of 2052 d and 0.00210.0002 d, respectively. The period variation would be produced by the light-travel-time effect due to a gravitationally-bound third body with a minimum mass of =0.76 M in an eccentric orbit of =0.61. This is consistent with the presence of third light found in our light-curve solution and the tertiary signal of 204.2 d period most likely arises from the K-type star crossed by the close eclipsing binary. Then, KIC002856960 is a triply eclipsing hierarchical system, A(BC), consisting of a close binary with two M-type dwarfs and a more massive K-type component. The presence of the third star may have played an important role in the formation and evolution of the close pair, which may ultimately evolve into a contact system by angular momentum loss.
19 pages, including 5 figures and 3 tables, accepted for publication in ApJ
References in corpus (8)
- Contact Binaries with Additional Components.I. The Extant Data
- KOI-126: A Triply-Eclipsing Hierarchical Triple with Two Low-Mass Stars
- The sdB+M Eclipsing System HW Virginis and its Circumbinary Planets
- Homogeneous studies of transiting extrasolar planets. II. Physical properties
- Reevaluating the Mass-Radius Relation for Low-Mass, Main Sequence Stars
- HD 181068: A Red Giant in a Triply-Eclipsing Compact Hierarchical Triple System
- KIC 4247791: A SB4 system with two eclipsing binaries (2EBs)
- Discovery of a double eclipsing binary with periods near a 3:2 ratio
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- TIC 114936199: A Quadruple Star System with a 12-day Outer Orbit Eclipse
- On the RZ Draconis Sub-stellar Circumbinary Companions Stability Study of the Proposed Sub-stellar Circumbinary System
- The Interior Structure Constants as an Age Diagnostic for Low-Mass, Pre-Main Sequence Detached Eclipsing Binary Stars
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