Please use this identifier to cite or link to this item: https://hdl.handle.net/11147/5290
Title: Triple-star candidates among the Kepler binaries
Authors: Rappaport, S.
Deck, K.
Levine, A.
Borkovits, T.
Carter, J.
El Mellah, I.
Sanchis-Ojeda, R.
Kalomeni, Belinda
Keywords: Binaries
Stars
Kepler binaries
Celestial mechanics
Eclipsing
Issue Date: May-2013
Publisher: IOP Publishing Ltd.
Source: Rappaport, S., Deck, K., Levine, A., Borkovits, T., Carter, J., El Mellah, I., Sanchis-Ojeda, R., and Kalomeni, B. (2013). Triple-star candidates among the Kepler binaries. Astrophysical Journal, 768(1). doi:10.1088/0004-637X/768/1/33
Abstract: We present the results of a search through the photometric database of Kepler eclipsing binaries looking for evidence of hierarchical triple-star systems. The presence of a third star orbiting the binary can be inferred from eclipse timing variations. We apply a simple algorithm in an automated determination of the eclipse times for all 2157 binaries. The "calculated" eclipse times, based on a constant period model, are subtracted from those observed. The resulting O-C (observed minus calculated times) curves are then visually inspected for periodicities in order to find triple-star candidates. After eliminating false positives due to the beat frequency between the ∼1/2 hr Kepler cadence and the binary period, 39 candidate triple systems were identified. The periodic O-C curves for these candidates were then fit for contributions from both the classical Roemer delay and so-called physical delay, in an attempt to extract a number of the system parameters of the triple. We discuss the limitations of the information that can be inferred from these O-C curves without further supplemental input, e.g., ground-based spectroscopy. Based on the limited range of orbital periods for the triple-star systems to which this search is sensitive, we can extrapolate to estimate that at least 20% of all close binaries have tertiary companions. © 2013. The American Astronomical Society. All rights reserved..
URI: http://doi.org/10.1088/0004-637X/768/1/33
http://hdl.handle.net/11147/5290
ISSN: 0004-637X
Appears in Collections:Physics / Fizik
Scopus İndeksli Yayınlar Koleksiyonu / Scopus Indexed Publications Collection
WoS İndeksli Yayınlar Koleksiyonu / WoS Indexed Publications Collection

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