Then and now: A new look at the eclipse timing variations of hierarchical triple star candidates in the primordial Kepler field, revisited by TESS

Open Access

Fig. 7.

Mass of the tertiary star, m_C, plotted against the binary mass, m_AB. Only LTTE + DE solutions were considered – the faint grey circles are the uncertain LTTE + DE systems. The blue line marks the q₂ = 1 boundary.

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