Von Zeipel - Lidov - Kozai cycles in action: $Kepler$ triples with eclipse depth variations: KICs 6964043, 5653126, 5731312 and 8023317
We report the results of the photodynamical analyses of four compact, tight triple stellar systems, KICs 6964043, 5653126, 5731312, 8023317, based largely on $Kepler$ and $TESS$ data. All systems display remarkable eclipse timing and eclipse depth variations, the latter implying a non-aligned outer...
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Main Authors | , , , , , |
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Format | Journal Article |
Language | English |
Published |
12.07.2022
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Subjects | |
Online Access | Get full text |
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Summary: | We report the results of the photodynamical analyses of four compact, tight
triple stellar systems, KICs 6964043, 5653126, 5731312, 8023317, based largely
on $Kepler$ and $TESS$ data. All systems display remarkable eclipse timing and
eclipse depth variations, the latter implying a non-aligned outer orbit.
Moreover, KIC 6964043 is also a triply eclipsing system. We combined
photometry, ETV curves, and archival spectral energy distribution data to
obtain the astrophysical parameters of the constituent stars and the orbital
elements with substantial precision. KICs 6964043 and 5653126 were found to be
nearly flat with mutual inclinations $i_{mut}=4.1$ deg and $12.3$ deg,
respectively, while KICs 5731312, 8023317 ($i_{mut}=39.4$ deg and $55.7$ deg,
respectively) are found to lie in the high $i_{mut}$ regime of the von
Zeipel-Kozai-Lidov (ZKL) theorem. We show that currently both high inclination
triples exhibit observable unusual retrograde apsidal motion. Moreover, the
eclipses will disappear in all but one of the four systems within a few
decades. Short-term numerical integrations of the dynamical evolution reveal
that both high inclination triples are currently subject to ongoing, large
amplitude ($\Delta e\sim0.3$) inner eccentricity variations on centuries-long
timescales, in accord with the ZKL theorem. Longer-term integrations predict
that two of the four systems may become dynamically unstable on $\sim$ Gyr
timescales, while in the other two triples common envelope phases and stellar
mergers may occur. Finally we investigate the dynamical properties of a sample
of 71 KIC/TIC triples statistically, and find that the mutual inclinations and
outer mass ratios are anti-correlated at the 4$\sigma$ level. We discuss the
implications for the formation mechanisms of compact triples. |
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DOI: | 10.48550/arxiv.2207.05517 |