论文标题
行星，单个M矮人和二元星伴侣的稳定性，以开普勒超脱二进制和可能的五个车身系统
Stability of planetary, single M dwarf, and binary star companions to Kepler detached eclipsing binaries and a possible five body system
论文作者
论文摘要
在这项研究中，我们确定了11个开普勒系统（KIC 525552、5653126、5731312、7670617、7821010、8023317、10268809、10296163、10296163、11519226、11558882和123356914 flip-inter Inter Inter Inter Inter Inter Inter Inter Inter Inter Inter Inter In系统的O-C图，报告这些系统的共同点以及这些系统是否动态稳定。这些系统以前已经报道了具有高度偏心的第三身体/外部伴侣的高偏心二元恒星。我们发现系统中的所有其他物体在先前报告的配置方面都是动态稳定的，因此很可能如所述存在。我们还提供了KIC5255552的其他证据，这是一个四颗星系统，该系统由黯然失色的二进制对和非移动的二进制对组成，并可能在系统中有第五个身体。随着NASA TESS系外行星的出现，其精确的光度监测提供了一个机会，可以帮助确认包括行星在内的更多当地黯然失色的二进制明星伴侣。
In this study we identify 11 Kepler systems (KIC 5255552, 5653126, 5731312, 7670617, 7821010, 8023317, 10268809, 10296163, 11519226, 11558882 and 12356914) with a "flip-flop" effect in the eclipse timing variations O-C diagrams of the systems, report on what these systems have in common and whether these systems are dynamically stable. These systems have previously reported high eccentric binary stars with highly eccentric third bodies/outer companions. We find that all of the additional bodies in the system are dynamically stable for the configurations previously reported and are therefore likely to exist as described. We also provide additional evidence of KIC5255552 being a quadruple star system comprised of an eclipsing binary pair and non-eclipsing binary pair with the possibility of a fifth body in the system. With the advent of the NASA TESS exoplanet survey, its precision photometric monitoring offers an opportunity to help confirm more local eclipsing binary star companions, including planets.
